The galaxy presents as a relatively smooth, elliptical-like object. It exhibits a centrally concentrated brightness profile, appearing to have a bright, well-defined core. The color gradient suggests a population of older stars dominating the core region, with a yellowish-white hue. A slight reddening is observed in the inner regions, possibly due to dust or a metal-rich stellar population. There is little evidence of distinct spiral arms or other features indicative of active star formation in the disk, if one exists. The galaxy seems to have a fairly uniform structure, appearing mostly undisturbed. The outer edges fade gradually into the background sky, with no apparent tidal features or signs of ongoing mergers.
