The galaxy appears to be a relatively bright, yellowish-orange object. Its morphology is generally smooth, lacking prominent spiral arms or a distinct disk. The light distribution suggests a centrally concentrated profile, with the brightest region located at its core. While mostly smooth, there may be some subtle disturbances or irregularities in its outer regions indicating a potential interaction or past merger event. The galaxy has a moderate roundness, showing a slight deviation from a perfectly spherical shape. There is a noticeable redder hue in the central region, possibly indicative of an older stellar population or dust obscuration. The overall color and smoothness suggest that the galaxy is likely an elliptical or lenticular type.
