The galaxy appears to be a relatively smooth, elliptical galaxy, possibly an E4 or E5 on the Hubble scale, showing moderate ellipticity. The central bulge is prominent and exhibits a bright, concentrated luminosity profile suggesting a high stellar density. The overall color appears yellowish, indicating an older stellar population with a lower rate of current star formation. No obvious dust lanes or spiral arm structures are visible. There is a slight indication of a fainter, more diffuse halo surrounding the brighter central region, which could be a population of older, more metal-poor stars. No signs of any major disturbances, such as tidal tails or distortions suggesting a recent merger event are readily apparent. The galaxy seems relatively isolated and undisturbed.
