The galaxy presents a predominantly smooth, elliptical morphology. There is little discernible spiral structure or evidence of active star formation within the main body of the galaxy, as indicated by its overall color profile. The central region appears brighter and slightly more yellow in comparison to the outer regions, possibly indicating an older stellar population concentrated towards the core. While the galaxy appears mostly undisturbed, there is a subtle asymmetry in the halo, potentially suggesting past interaction or minor disturbance, although no significant tidal tails or signs of a major merger are immediately apparent. The galaxy exhibits a generally intermediate ellipticity, not appearing particularly round nor cigar-shaped.
