The galaxy presents as an elliptical morphology with a high degree of central concentration. It exhibits a smooth, featureless profile, lacking distinct spiral arms or prominent dust lanes. A bright, unresolved central bulge dominates the luminosity, suggesting a substantial population of older stars. The overall color index indicates a relatively blue hue within the central region, transitioning to redder tones in the outer halo. There are some indicators of a possible minor disturbance or interaction event based on asymmetries within the disk. Faint extensions are visible on the outer edges of the galaxy, suggesting possible tidal features or past mergers. However, the strong central brightness limits detailed observations of any fainter structures.