The galaxy presents a roughly elliptical morphology, appearing somewhat compact. A bright, relatively well-defined central core region is observed. Fainter, diffuse material extends outward from the central region. The color profile indicates variations across the galaxy's structure, trending from red towards the outer edges to blue in the center. There appears to be a minor disturbance visible at the edge of the galaxy. The smooth, featureless appearance indicates a low probability of spiral arm structure or significant dust lanes, suggesting a relatively homogenous stellar population distribution. The object does not appear to be undergoing a major merging event, though a minor disturbance could signify interaction with another celestial body.
