The galaxy appears as a lenticular or early-type spiral system, exhibiting a generally smooth, diffuse profile with a moderate degree of central concentration. There is a subtle elongation present, but without any apparent spiral arm structure or prominent disk features discernible. The color gradient suggests a population dominated by older stars, exhibiting a yellowish-orange hue. There is no indication of ongoing, significant star formation regions from the color. The object does not exhibit any clear evidence of tidal disturbances or interaction with other galaxies. The object has a moderate size. 
