The galaxy presents as a single, somewhat diffuse object with a smooth, elliptical morphology. The core exhibits a bright, concentrated luminosity, suggesting a dense stellar population. The color gradient is subtle, showing a tendency toward redder hues in the central region, potentially indicating older stellar populations, and slightly bluer hues towards the periphery. There is no apparent spiral structure or significant dust lane visible. The galaxy does not show strong signs of tidal interaction or major disturbance. The overall appearance indicates an evolved system, possibly an elliptical galaxy undergoing passive evolution.
