The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy. It exhibits a concentrated central bulge that displays a yellowish hue, suggestive of an older stellar population. The galaxy is not perfectly round, with a slight elongation along one axis. There is little evidence of spiral arm structure or prominent dust lanes, giving it a generally featureless appearance. The outer regions of the galaxy gradually fade into the background, showing no sharp edges. The overall color gradient suggests a higher concentration of older, redder stars towards the center, and a possibly younger population in the surrounding areas. There does not appear to be any ongoing major merging activity or tidal disturbances.
