The galaxy presents as a central bulge that appears largely spheroidal and exhibits a yellowish-white hue, suggestive of an older stellar population. This galaxy appears to be at an intermediate redshift, likely at a distance requiring light to have traveled for a significant fraction of the universe's age to reach our instruments. Faint disk-like features are observed emanating from the bulge. These features are not well defined, as they seem disturbed. The light is blueish, a possible indication of active or recent star formation. One side of the galaxy has an especially prominent redder area, possibly indicating a particularly active zone of star formation with a high concentration of dust. The morphological classification appears to lean toward a relatively smooth structure overall, with some disturbances and faint features indicative of a disk. The overall shape of the galaxy falls between being perfectly rounded and cigar-shaped, and it displays signs of potentially minor disturbances but with a notable fraction of observations suggesting no apparent merging activity. The estimated stellar mass of the galaxy is considerable, classifying it as a relatively massive galaxy. Star formation rate is detectable, potentially being in a transition stage. The galaxy is likely in a phase between forming stars at a high rate and quiescence, a process during which star formation slows down and eventually ceases.
