The galaxy presents as a singular, relatively compact object. It exhibits a smooth morphology, with no immediately discernible spiral arms or bar structure. The overall shape is elliptical or spheroidal, leaning towards rounded rather than elongated. There is a slight suggestion of a brighter central region, possibly indicating a concentrated nucleus or bulge. The color profile appears relatively uniform across the galaxy, with a yellowish hue that suggests a stellar population dominated by older, redder stars. There is no obvious evidence of active star formation regions or significant dust lanes. There is no major evidence of any ongoing major merging activity or tidal disturbances, though some minor disturbance cannot be ruled out from the image alone.
