The galaxy presents as a fairly smooth, elliptical-like structure. The core region exhibits a concentrated, bright luminosity suggesting a high density of stars within the central bulge. Moving outward from the core, the light gradually diminishes into what appears to be a more diffuse halo. There is a color gradient; the core leans towards yellow-red, indicating an older stellar population. The surrounding region is slightly bluer, suggesting the presence of younger, hotter stars, although star formation activity is not strongly evident in this image. The overall morphology implies that this system is in a relatively stable, post-starburst stage. There is no obvious dust lane or spiral arm structure. Overall, the galaxy appears largely undisturbed with no obvious signs of tidal features or ongoing major mergers. It has a round shape, it is a very compact galaxy. 