The galaxy presents as a somewhat elliptical, diffuse object. A significant fraction of its light appears concentrated in a central region. The overall color profile suggests an older stellar population, with a slight bluer tint in the central area indicating the possible presence of some younger, hotter stars. The galaxy appears relatively smooth, lacking prominent spiral arms or significant dust lanes. No obvious signs of a major merger event are apparent, although some minor disturbance cannot be ruled out. The galaxy exhibits a faint, extended halo. The ratio of semi-major to semi-minor axis is approximately .95, close to a circular galaxy. Based on the observed color and morphology, this object appears to be an early-type galaxy.
