The galaxy exhibits a generally elliptical morphology, appearing largely smooth and relatively undisturbed. The light profile suggests a centralized concentration, with the highest intensity emanating from the core. The object displays a color gradient from a central yellowish-white hue, shifting towards a redder tint towards the edges. The galaxy has an apparent angular size of approximately 4 arcseconds, indicating it is not a particularly nearby object. There is little indication of active star formation from this image alone; the smooth profile and color distribution suggest a population dominated by older stars. The galaxy does not appear to be undergoing a major merger or experiencing significant tidal disruption.
