The galaxy appears to be a relatively compact system, approximately 2 kpc in radius. The morphology is predominantly smooth and elliptical in nature. The light distribution suggests a bulge-dominated structure. The galaxy exhibits a bright central region, indicative of a concentrated nucleus or core. The color gradient suggests a redder core transitioning to slightly bluer outer regions. There is subtle evidence of asymmetry in the galaxy's overall shape, but this is not indicative of a major merger or significant tidal disruption. There is also a hint of a spiral arm structure. Overall, the galaxy appears to be a relatively massive system with a low rate of star formation.
