The galaxy presents as a somewhat elliptical structure, with a smooth, diffuse appearance. Its color profile suggests a mixed stellar population, exhibiting a central concentration with a subtle reddish hue, possibly indicating the presence of older, redder stars within the bulge. The outer regions of the galaxy display a slightly bluer tint, which could be indicative of more recent star formation activity. While a distinct disk is not readily apparent, a subtle flattening suggests it is likely of a lenticular type galaxy, but also could be an elliptical galaxy. No prominent spiral arms or dust lanes are discernible in this image. The overall morphology suggests a relatively evolved system that is most likely a galaxy that is either an elliptical or lenticular. There is no indication of strong tidal interactions or major mergers, with a relatively undisturbed appearance.
