The galaxy presents as an elliptical structure, with a smooth, diffuse light distribution. There is a noticeable concentration of light towards the center, indicating a likely bulge component. The overall color is on the redder end of the spectrum, suggesting a population of older stars. There is little to no indication of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, with no obvious signs of recent mergers or tidal interactions. Its morphology appears generally smooth and spheroidal. The isophotes appear fairly regular and concentric. Based on the observed characteristics, the galaxy appears to be an early-type galaxy dominated by older stellar populations.
