The galaxy presents a generally smooth and elliptical morphology. It exhibits a concentrated central bulge that appears yellowish-orange, suggesting a population of older stars. There is no discernible spiral arm structure or prominent dust lanes. The overall shape is predominantly round, with a slight deviation toward an intermediate form. No major merger events are apparent, though subtle asymmetries might indicate minor disturbances or tidal interactions. The galaxy is relatively compact, with a measured radius. The color gradient suggests a possible ongoing, but low, rate of star formation.
