The galaxy presents an overall elliptical morphology, with a smooth, centrally concentrated luminosity profile. The core region exhibits a bright, yellowish-white hue, potentially indicative of an older stellar population and/or ongoing star formation in the galactic nucleus. The galaxy extends outward from the core, transitioning to fainter, bluish hues. There is some indication of a slight disk-like structure but this is not prominent. The smooth appearance and lack of strong tidal features suggest that the galaxy is relatively undisturbed, and possibly an early-type galaxy. There is a slight asymmetry in the outer regions, which may point to a minor gravitational interaction or past merger event.