The galaxy presents as a relatively smooth, elliptical structure with a discernible central bulge. The core region exhibits a bright, concentrated luminosity, suggesting a high density of stars. The overall color gradient transitions from a yellowish-white in the core to a bluer hue in the outer regions, possibly indicating a younger stellar population in the galactic halo or disk. A slight elongation is observed, with a minor asymmetry in the outer regions, which could be indicative of a past minor disturbance or interaction, however it appears mostly relaxed. There is no apparent dust lane or spiral arm structure visible.
