The galaxy presents as a primarily smooth, elliptical-like structure. The central region exhibits a high concentration of light, appearing significantly brighter and yellower than the outer regions, possibly indicative of an older stellar population. There may be three distinct nuclei, indicating a possible merger event. Faint, diffuse extensions are barely visible. The overall color suggests a relatively low rate of ongoing star formation. The general morphology seems to lean towards a more spheroidal shape.
