The galaxy presents as a centrally concentrated, relatively smooth object. The core region exhibits a bright, somewhat diffuse appearance with a yellow-white hue. The overall shape is ellipsoidal, appearing almost perfectly in between round and cigar-shaped, suggesting a possible oblate spheroid structure. A faint, blue-ish, extended feature or possible arm is visible on one side, possibly indicating minor disturbances or interaction. The galaxy lacks prominent spiral arms or significant dust lanes. The smooth appearance, combined with the color profile, indicates a significant population of older stars, and a low ongoing star formation rate. A slight redward color shift from core to edges is present, indicating possible population gradients. Overall, the galaxy appears to be a relatively undisturbed, intermediate mass system, transitioning towards a more quiescent phase of galactic evolution.
