The galaxy appears as a relatively small, faint, and somewhat elongated object. Its central region exhibits a smooth, concentrated light distribution, suggesting a dominant bulge component. There is a subtle disk feature, indicated by the slight elongation and hints of structure extending from the central bulge, but the disk's features are not very prominent. The galaxy's color is moderately red, implying a population of older stars and a lower rate of ongoing star formation. There are no obvious signs of strong tidal interactions or major mergers, although minor disturbances cannot be ruled out due to the limited resolution. Overall, the galaxy presents as an intermediate type, potentially between an elliptical and a spiral, with a more bulge-dominated morphology.
