The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. The light distribution appears consistent across the galaxy, displaying a dominant central bulge. There may be a faint disk component, but it is not clearly resolved. The galaxy exhibits a redder color profile, possibly indicating an older stellar population. There is no strong evidence of spiral arms or significant star formation regions. The absence of tidal tails or other strong distortions suggests that the galaxy is not undergoing any major mergers or interactions, and that it appears generally undisturbed.
