The galaxy presents as a fairly smooth, concentrated object with an overall yellowish-orange hue. Its morphology appears elliptical, exhibiting a high degree of radial symmetry. There are no obvious spiral arms, bars, or significant dust lanes visible. The light profile suggests a concentrated central region that gradually fades outward, consistent with a spheroidal galaxy type. There are no indications of strong tidal interactions or mergers. The galaxy's color suggests a relatively old stellar population, typical of early-type galaxies, and a low rate of star formation. Based on its overall appearance, the object is likely a massive elliptical galaxy.
