The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated bulge with a gradual decrease in luminosity towards the outer regions. The color profile suggests a dominant population of older stars, indicated by the yellowish-red hue, particularly prominent in the core. There's a subtle hint of bluer tones in the outer regions that may indicate the presence of some younger stars. The isophotes are generally smooth, and only slight disturbances can be detected in the structure, meaning it is not undergoing major merging activity. Given the smooth appearance and color profile, this galaxy is potentially an early-type galaxy, possibly an elliptical or lenticular type, at a distance of roughly 6.5 kpc in radius.
