The galaxy presents as a relatively smooth, elliptical morphology. A concentrated central bulge is evident, exhibiting a yellowish-white hue, suggesting a population of older stars. The outer regions of the galaxy fade into a less defined halo. There is no discernible disk structure or spiral arms. The overall shape is somewhat elongated but not significantly cigar-shaped. There are no obvious signs of a major merger or significant tidal disturbances, and the structure appears largely undisturbed.
