The galaxy appears as a relatively smooth, elliptical-like object. It exhibits a concentrated central bulge, with a gradual decrease in surface brightness outwards. The color profile is generally yellowish, suggesting a population of older stars. There's a hint of a very subtle disk feature, though the overall morphology leans heavily toward an early-type galaxy classification. No significant signs of ongoing star formation are readily apparent, aligning with a passively evolving system dominated by older stellar populations. There is no obvious sign of any major disturbance or ongoing merging activity. The galaxy appears relatively isolated and undisturbed.
