The galaxy presents as a centrally concentrated elliptical system. It exhibits a smooth, diffuse light distribution, lacking any discernible spiral arm structure or prominent dust lanes. There is no indication of a central bar. The morphology appears largely undisturbed, showing no signs of a major merger event. The galaxy appears roughly rounded in shape. There may be minor disturbance in the surrounding galactic halo. The galaxy appears to be an early type galaxy, and given the color, may have a large population of older stars.
