The galaxy presents as a smooth, elliptical-like structure, with a moderately elongated morphology. Its core region exhibits a concentrated, brighter luminosity, possibly indicating a high stellar density. The color profile is predominantly reddish-yellow, suggesting a population of older stars. Faint greenish hues are observed in the outer regions, potentially indicative of ongoing, though relatively subdued, star formation activity. No prominent spiral arms or distinct dust lanes are discernible, supporting the overall smooth classification. There is no indication of a major ongoing merger, though the slightly irregular shape suggests it may be a merger remnant or be undergoing minor tidal disturbance. The overall structure appears relatively undisturbed.
