The galaxy presents as a relatively compact, elliptical-like structure, though not perfectly spherical. Its core exhibits a concentrated, bright yellowish-orange color, suggestive of an older stellar population. There's a subtle gradation outward from the core, indicating a gradual decrease in stellar density. The outer regions appear more diffuse. No distinct spiral arm structure or prominent dust lanes are visible. There's also no evidence of any on-going major merger event. The overall smooth appearance indicates it is likely dominated by an older stellar population with a possible low star formation rate.
