The galaxy presents as a centrally concentrated, elliptical-like structure. It exhibits a smooth, relatively featureless profile, with a noticeable radial gradient in luminosity, brightest at the core and gradually diminishing outwards. There is very little to no discernible dust lane obscuration or distinct spiral arm structure. The galaxy appears slightly elongated. The color gradient suggests a population of older stars, with a relatively redder overall hue. There is no evidence of an ongoing major merger.
