The galaxy presents a somewhat rounded morphology, appearing more like a transitional elliptical or a spiral galaxy viewed face-on with minimal discernible spiral arm structure. The central bulge exhibits a concentration of light, suggesting a population of older stars. The surrounding disk, if present, is fainter and blends into the background, implying a lower surface brightness. There may be some slight disturbances in its form, though nothing major. Overall, this galaxy appears to have a smooth texture, with a general absence of strong star-forming regions. Its color suggests a relatively evolved stellar population.
