The galaxy presents as a centrally concentrated object with a smooth, diffuse light profile. There is a lack of apparent spiral arm structures or prominent dust lanes, suggesting a generally featureless morphology. The color appears yellowish, possibly indicating an older stellar population and/or significant dust obscuration. The observed roundness implies a low inclination angle with respect to the observer. Based on the absence of strong tidal features or multiple nuclei, the galaxy appears to be relatively undisturbed by major merger events. There may be a smaller, faint object in close proximity to the bottom left of the galaxy that is likely a background galaxy, however, a deeper image would be needed to clarify the morphology of that galaxy.