The galaxy presents as a centrally concentrated elliptical, exhibiting a smooth, diffuse light profile characteristic of an early-type system. The apparent ellipticity is moderate, suggesting a somewhat flattened spheroidal shape. The color gradient appears subtle, with a slightly redder hue towards the galactic center, potentially indicative of an older stellar population dominating the core. There are no readily discernible spiral arms, dust lanes, or other features associated with ongoing star formation. The galaxy appears relatively undisturbed, lacking evidence of recent mergers or tidal interactions. The estimated size is relatively small, but this could be due to distance. Overall, the morphology is consistent with a quiescent elliptical galaxy.
