The galaxy presents as a moderately bright, elongated structure. The central region exhibits a higher luminosity, appearing nearly spheroidal. The overall color profile suggests a population of older stars dominating the core. The outer regions show a somewhat bluer hue, which hints at ongoing, albeit modest, star formation. The morphology appears to be relatively smooth. There may be some slight disturbance evident in the outer reaches of the galaxy, but it is not distinct. It could be an elliptical type, or a spiral seen at an angle.
