The galaxy presents as a relatively luminous, though somewhat diffuse, object. Its morphology appears to be predominantly smooth, with a notable central bulge that exhibits a yellowish hue, suggesting a concentration of older stellar populations. The outer regions of the galaxy fade gradually, displaying a bluer tint. The overall shape is moderately elliptical. There is a hint of possible disk structure, but no defined spiral arms are readily apparent. There is a minor indication of disturbance in the surrounding area, but the galaxy itself appears largely undisturbed with no major ongoing mergers. The galaxy could be a large and massive spiral, or it could be a moderately massive elliptical galaxy. It is actively forming stars at a low rate.