The galaxy appears to be a relatively smooth, elliptical type. It exhibits a concentrated central bulge that is bright and slightly yellowish, suggesting an older stellar population. The outer regions of the galaxy fade into a diffuse halo with a bluish tint, potentially indicating some presence of younger, bluer stars. The overall shape is more rounded than elongated, and the lack of distinct spiral arms or a prominent disk structure is noticeable. There is some indication of minor disturbances or irregularities in the outer regions, but no obvious signs of a major merger or strong tidal interactions. Based on its morphology, this galaxy appears to be a passively evolving system with a moderate amount of stellar mass and a low rate of ongoing star formation.
