This galaxy exhibits a relatively smooth morphology, appearing somewhat elongated in shape, but not extremely so. The central bulge is prominent and displays a yellowish hue, suggesting a population of older stars. Fainter, bluer light is present in the surrounding disk, hinting at some ongoing star formation, though the overall color indicates that star formation is not dominant. There are hints of some spiral structure in the disk, but these features are not sharply defined, giving the galaxy a somewhat diffuse appearance. There is no clear indication of major mergers or strong tidal disturbances. The overall impression is of an intermediate-mass galaxy transitioning from a more actively star-forming state to one dominated by an older stellar population.
