The galaxy presents an elliptical morphology, exhibiting a predominantly smooth structure. The central region is noticeably brighter, concentrated in a yellowish hue indicating an older stellar population. The light gradually diminishes towards the outer edges of the galaxy, but no distinct spiral arms or disk-like features are discernible. The overall shape of the galaxy is largely spherical in appearance with only slight elongations visible. There appears to be no significant interaction or major disturbance evident in the galaxy's structure. The galaxy’s appearance suggests it may have undergone past mergers, leading to its relatively smooth structure. Faint outer regions of this galaxy are visible, extending beyond its more luminous core, potentially indicating the presence of a stellar halo.
