The galaxy presents as a relatively compact object, displaying a smooth, elliptical morphology. The light distribution appears concentrated towards the center, with a gradual decrease in brightness towards the outer edges, suggesting a lack of distinct spiral arm structures. The shape is notably elongated, exhibiting a cigar-like appearance. There is no strong evidence of ongoing major mergers or significant tidal disturbances; however, a very slight asymmetry in the outer halo cannot be ruled out as potential signs of minor interactions. The overall color of the galaxy is a subdued blue-white, suggestive of a stellar population that is not dominated by very old red stars, but may not include high rates of current star formation.
