The galaxy presents as a yellowish-orange elliptical-type system. It displays a smooth, featureless morphology without prominent spiral arms or a distinct disk structure. The galaxy appears elongated, exhibiting an axis ratio indicative of an E4-E5 classification on the Hubble sequence. A bright central bulge dominates the luminosity profile, with the light appearing to gradually fade toward the outer edges, suggesting a high degree of central concentration. The absence of blue colors implies a dearth of ongoing, significant star formation within the galaxy.
