The galaxy presents an elliptical morphology with a relatively smooth structure. The core of the galaxy exhibits a bright, concentrated luminosity suggesting a high stellar density. Moving outward from the core, the light gradually diminishes, forming a diffuse halo. The galaxy appears generally rounded, although there is a slight elongation or asymmetry visible on the lower side. The colors indicate that the galaxy is likely composed of an older stellar population, with a reddish-yellow hue dominating. There is little evidence of significant dust lanes or spiral arm structures. This galaxy does not display any signs of major disturbances, and the structure appears relatively relaxed.
