The galaxy appears to be a relatively smooth, elliptical-type galaxy, possibly an S0. It exhibits a concentrated central bulge region with a noticeable decrease in luminosity moving outwards towards the edges. The core exhibits a reddish hue, suggestive of an older stellar population. Surrounding the core, there is a broader, fainter halo region with a slightly bluer tint, which could indicate more recent star formation, although at a low rate. The overall structure indicates that the galaxy is fairly relaxed, with no significant signs of recent major mergers or strong tidal disturbances. The galaxy appears to be of intermediate size, with the halo region gradually fading into the background sky.
