The galaxy presents a roughly elliptical morphology, appearing predominantly smooth with a concentrated central bulge. Faint, diffuse extensions are observable surrounding the central region, hinting at a possible disk or halo structure. The color distribution suggests an older stellar population in the bulge, indicated by the yellowish-red hue, while bluer colors are seen in the outer regions, potentially signifying ongoing star formation, albeit at a moderate rate. There are hints of minor irregularities or disturbances in the outer regions, possibly suggesting past interactions or mergers. No prominent spiral arm structures are discernible. The galaxy exhibits an intermediate redshift, classifying it as a distant object. Overall, the galaxy seems to be a moderately massive system, exhibiting characteristics of both elliptical and spiral galaxies, potentially undergoing a transitional phase in its evolutionary pathway.
