The galaxy appears to be a relatively compact, elliptical galaxy. Its central region exhibits a bright, concentrated core, suggesting a high density of stars or potentially an active galactic nucleus, however, its color does not support a large amount of activity. The overall shape is nearly round, with a slight elongation that distinguishes it from being perfectly spherical. There's a noticeable smoothness to its structure, indicating a lack of prominent spiral arms or significant dust lanes. The galaxy displays a color gradient, shifting from a bluer hue in the central region to a redder, more diffuse halo. This may suggest ongoing star formation in the nucleus, and older, redder stars in the outer regions. There is no obvious evidence of any major merging events or tidal disturbances in the galaxy's vicinity.
