The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated central bulge, which dominates the overall light profile. There is a gradual decrease in luminosity moving outward from the core. The color gradient suggests an older stellar population. The smooth morphology implies a lack of significant recent mergers or major disturbances, although some minor asymmetries are noted. The galaxy is relatively round, showing a slightly elongated shape but not strongly cigar-shaped. There is no visible spiral arm structure, dust lanes, or prominent star-forming regions. The overall appearance is indicative of a relatively quiescent galaxy with low star formation activity.