The subject galaxy presents as a relatively small, elongated object. Its morphology appears primarily smooth with a slight central condensation in surface brightness. The light distribution suggests a prolate spheroidal shape, potentially indicative of an elliptical or lenticular galaxy. There is a subtle hint of a disk-like structure, but it does not contribute significantly to the overall morphology. Faint, reddish hues permeate the galaxy. The overall structure seems undisturbed, showing no clear evidence of ongoing major merger events or tidal features.
