The galaxy presents a generally smooth, elliptical morphology. The core is a bright, concentrated region, exhibiting a yellowish-white hue. The isophotes appear mostly regular, but there is a very slight deviation toward a cigar shape. The outer regions of the galaxy fade gradually into the background sky, suggesting a lack of distinct spiral arms or significant tidal features. There are no obvious signs of recent or ongoing major merger activity, although there could be a minor disturbance. The overall color suggests a stellar population dominated by older stars, which implies a relatively low star formation rate.
