This galaxy exhibits an overall elliptical morphology. The central region presents a bright, concentrated core, suggesting a high density of stars or potentially an active galactic nucleus. A diffuse halo surrounds the central region, displaying a gradient of decreasing luminosity outwards. This indicates a gradual decline in stellar density away from the galactic center.

There is evidence of structural irregularities or disturbances. Subtle features such as faint, asymmetrical extensions or tidal tails can be observed. These features suggest recent or ongoing gravitational interactions with other galaxies or smaller satellite objects. Furthermore, there appears to be a degree of color variation across the galaxy, with some regions exhibiting bluer hues, indicative of younger stellar populations, and other regions displaying redder hues, suggestive of older stellar populations. This galaxy lacks any definitive spiral arm structure, which further supports the classification as an elliptical galaxy, albeit one that may have experienced recent mergers or tidal interactions.
