The galaxy presents as a moderately luminous, relatively compact object with a dominant elliptical morphology. It exhibits a smooth, centrally concentrated luminosity profile, indicating a high degree of spheroidal symmetry. There is a hint of a flattened shape, leaning towards an oblate spheroid.

Color gradients are subtle but present. The core region appears to be characterized by a yellowish-white hue, suggesting a population of older stars. Moving outward from the core, a slight bluish tint emerges, which could indicate the presence of a younger stellar population, though not substantially so. There is no clear evidence of distinct spiral arms or prominent dust lanes. Any potential features that could support a classification other than elliptical appear to be subdued. Given its distance, and based on the observed color and smoothness, it is plausible that the galaxy is an early-type galaxy undergoing moderate levels of star formation. Based on the smooth shape, this is most likely an elliptical galaxy.
