The galaxy presents as a relatively compact, somewhat elliptical object. The light profile appears smooth and centrally concentrated, exhibiting a roughly spherical shape. There is a suggestion of a slight elongation or departure from perfect circularity.

The color distribution is not uniform; a possible gradient is visible, with the central region appearing bluer and the outer edges trending towards redder hues. This may suggest a younger stellar population concentrated in the core, with older stars dominating the outskirts.

Evidence of significant structural features, such as spiral arms or a prominent disk, is absent. Subtle irregularities in the outer regions, such as faint plumes, may be indicative of past minor interactions or internal dynamical processes. However, these features are not pronounced. The overall appearance is consistent with an early-type galaxy, possibly an elliptical or lenticular galaxy.
