The galaxy presents as a somewhat elliptical, concentrated object with a smooth morphology. Its central region exhibits a bright, yellowish hue, suggestive of a population of older stars, potentially with a significant contribution from a bulge component. The outer regions appear fainter and more diffuse, indicating a gradual decrease in stellar density away from the center. There is a faint disk structure component and the roundness of this galaxy looks in between a true circle and a cigar shape. There is no indication of strong star formation. The galaxy does not obviously appear to be undergoing any major merging activity or significant tidal disturbances; it seems generally undisturbed.
