The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a concentrated, bright luminosity suggesting a significant stellar density. Progressing outwards from the core, the galaxy gradually diminishes in brightness, forming a diffuse halo with no distinct features such as spiral arms or prominent dust lanes. The color profile indicates a higher concentration of older stars, particularly towards the center, which appears yellowish-orange. There is very faint bluer light in the outer halo, suggesting a small amount of ongoing or recent star formation, but the dominant population is likely composed of older, redder stars. The overall structure indicates it is unlikely to be undergoing any major mergers or tidal disturbances and it seems relatively undisturbed. The apparent roundness of the object supports its classification as an elliptical galaxy.
