The galaxy presents as an elliptical or lenticular type with a smooth, centrally concentrated luminosity profile. It exhibits a flattened shape. The galaxy's light distribution is elongated, with a major axis significantly longer than its minor axis. A minor disturbance within the galaxy suggests a potential for previous interaction. The central region displays a higher concentration of luminosity, indicating a possible bulge component. The overall color is relatively blue, perhaps indicating moderate ongoing star formation. The galaxy appears relatively isolated.