This galaxy exhibits an overall elliptical morphology. The core region is bright and concentrated. Surrounding the core, there is a diffuse, less luminous halo, suggestive of an extended stellar population. A flattened disk is observable around the core; it seems to have a slight vertical bulge at the center. No distinct spiral arm structures are visible. The galaxy exhibits a gradient of color, with the core and inner disk appearing bluer. This could indicate a region of active star formation. The outer halo appears redder in comparison, indicative of an older stellar population. There is no strong evidence of tidal tails or other disturbances, indicating it is likely in its relaxation stage.