The galaxy presents as a somewhat smooth, centrally concentrated object. It exhibits a generally elliptical morphology, tending towards roundness, though with a slight elongation suggesting a weak disk-like structure. The galaxy's color profile indicates a redder hue, transitioning towards a yellower center, suggestive of an older stellar population dominating its composition. There is a possible sign of minor disturbances, but overall the galaxy appears relatively undisturbed.
