The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated morphology. The light profile suggests minimal structure, with no distinct spiral arms or prominent dust lanes visible. It displays a high degree of roundness and a fairly uniform color gradient across its body, suggesting a relatively old stellar population. The overall color is on the redder side, pointing towards a population dominated by older, redder stars and a likely suppression of ongoing star formation. There are no obvious signs of major mergers or tidal disturbances in the immediate vicinity, although a minor asymmetry or faint feature could be present upon closer inspection.
