The galaxy presents as a relatively smooth, elliptical-like structure, appearing mostly round in shape. The central region exhibits a concentrated luminosity, appearing bright and yellowish. Progressing outwards from the core, the intensity gradually diminishes, forming a diffuse halo. There are hints of fainter, bluish extensions along one edge, potentially suggesting some disk-like characteristics or tidal features. There is an indication of a minor disturbance in the form of a reddish area near the primary mass of the galaxy. Overall, the galaxy appears to be relatively isolated, showing no prominent signs of ongoing major mergers or interactions.
