The galaxy appears to be a relatively smooth, elliptical type, exhibiting a centrally concentrated luminosity profile. There is a distinct lack of spiral arm structure, and no prominent dust lanes are visible. The shape is roughly in between being round and cigar shaped. The galaxy's core is significantly brighter than its outer regions, suggesting a high concentration of stars in the nucleus. There are hints of a subtle color gradient, potentially indicating variations in stellar populations or metallicity. There is no evidence of major ongoing mergers or significant tidal disturbances, though there is the suggestion of minor disturbance.