The galaxy presents as a generally smooth, elliptical-like structure. Its color profile suggests a dominant population of older stars, indicated by the yellowish-orange hue concentrated toward the galaxy's core. There is a slight hint of a bluer color in the outer regions which may indicate some ongoing, but subdued, star formation. The overall symmetry is nearly circular, with only minor apparent deviations from a perfectly rounded shape. There are no clear signs of major disturbances or mergers, however there appears to be some subtle evidence of an interaction, possibly in the form of an unidentifiable minor disturbance to the overall symmetry. The lack of prominent spiral arms or a defined disk structure supports the classification as an early-type galaxy.
