The galaxy presents a generally elliptical morphology. Its light profile appears relatively smooth and centrally concentrated, with a gradual decline in surface brightness from the core outwards. There is no obvious disk component or spiral arm structure visible in this image. The primary color appears whitish, suggesting a stellar population dominated by older, less massive stars with a low rate of on-going star formation. Subtle color variations may be present, but the resolution limits detailed analysis of stellar populations or dust distribution. No prominent tidal features or signs of recent major merger activity are immediately apparent.
