The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology is largely elliptical, displaying a round, though not perfectly spherical, shape. A distinct nucleus appears bright, possibly indicating the presence of an active galactic nucleus or a high concentration of stars in the galactic core.

The overall color gradient suggests a dominant population of older stars, with a general reddish-yellow hue. Patches of bluer light are very subtly present, suggesting ongoing, but subdued, star formation. The galaxy does not exhibit any apparent signs of significant tidal disturbances or ongoing major mergers, though very minor irregularities in the outer regions hint at possible past interactions. There is no spiral arm structure or dust lane visible.
