The galaxy appears as a roughly elliptical, somewhat spheroidal object with a concentrated central bulge that dominates the overall luminosity. The core exhibits a yellowish-white hue, possibly indicating an older stellar population within. There's a faint greenish-blue tinge surrounding the central bulge, suggesting the presence of some younger, hotter stars or ionized gas, although this is not particularly pronounced.

A faint, diffuse disk component seems to be present, extending beyond the central bulge, but it lacks any distinct spiral arm structure. There may be a minor disturbance on one side of the galaxy, with some evidence of a faint, reddish region that could be a tidal feature or an area of active star formation resulting from a past interaction. This disturbance does not seem to heavily disrupt the main structure of the galaxy, suggesting that the galaxy is not currently undergoing a major merger. The overall morphology is relatively smooth, indicating a higher fraction of older stars and a more quiescent star formation rate.
