The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. The core region exhibits a bright, yellow-white hue, suggestive of an older stellar population. There is a very slight color gradient outwards from the core. The overall structure appears undisturbed, showing no obvious signs of a major merger or significant tidal interactions. Faint, diffuse extensions are possibly visible extending from the main body. The galaxy's roundness is pronounced, indicating a minimal degree of ellipticity.
