The galaxy presents as a relatively compact object with a smooth overall appearance. Its morphology is generally elliptical, exhibiting an intermediate roundness, not perfectly spherical but lacking a highly elongated or cigar-like shape. The light profile appears centrally concentrated with a gradual decrease in brightness towards the outer edges, indicative of an older stellar population. Faint color variations can be observed, with the central region appearing slightly more yellow or red in comparison to the outer regions, which are slightly bluer. No prominent spiral arms, distinct bars, or significant dust lanes are discernible. There is no obvious evidence of major mergers or significant tidal disturbances.
