The galaxy presents as a centrally concentrated object, approximately elliptical in shape, with a smooth, diffuse light distribution. There is no obvious spiral arm structure or significant dust lane obscuration visible. The core region appears brighter and more compact than the outer regions, which fade gradually into the background. There is a hint of tidal distortion, with what looks like a plume or tail visible. The galaxy's color appears slightly redder toward the core, suggesting an older stellar population.
