The galaxy presents as a relatively smooth, elliptical-like structure. The light is centrally concentrated and diffuse, with no distinct spiral arms or bar features visible. Color gradients across the galaxy are subtle, with a slightly bluer hue in the central region transitioning to redder tones outwards, suggesting a stellar population with a range of ages, with younger bluer stars in the core and older redder stars towards the edge. There is no obvious dust lane.
