The galaxy presents an overall elliptical morphology, appearing largely smooth and lacking prominent spiral arm structures. The central bulge is bright and concentrated, exhibiting a slightly yellowish-white hue, possibly indicative of an older stellar population. The outer regions of the galaxy fade into a bluish halo, which could suggest the presence of younger stars, perhaps formed through more recent star formation activity. The shape is generally in-between round and cigar-shaped. There is a subtle hint of disturbance or asymmetry in the galaxy's overall structure, suggesting a potential past interaction or minor disturbance. The galaxy's size is relatively compact.
