The galaxy presents as a relatively smooth, elliptical morphology. A bright central bulge dominates the structure, displaying a concentrated luminosity profile. Moving outward, the galaxy exhibits a gradual decrease in surface brightness, suggesting a fairly homogenous stellar population. There are no prominent spiral arms or distinct dust lanes visible. The overall color appears to be reddish, indicative of an older stellar population with lower ongoing star formation. Faint, diffuse, and irregular outer regions hint at possible tidal interactions or past minor mergers, but the core remains largely undisturbed. The galaxy appears mostly undisturbed.
