The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. There is a noticeable lack of distinct spiral arm structures or significant dust lanes. The light profile suggests it's largely spheroidal in shape, although there is some slight ellipticity. The color appears relatively uniform across the galaxy, trending towards a yellow/red hue, potentially indicating an older stellar population. The galaxy is roughly 3.5 kpc in radius. The object is consistent with a massive galaxy with a low rate of star formation and an estimated stellar mass exceeding 10^10 solar masses. There is no visible evidence of any major merging or tidal disturbances.
