The galaxy presents as a centrally concentrated object, appearing relatively smooth in texture. A slight elongation is discernible, with the major axis oriented approximately horizontally. A luminous, ochre-colored region dominates the central area, potentially indicative of an older stellar population or dust obscuration. Surrounding this central concentration is a bluer halo or disk-like component. There is a possible indication of faint, diffuse arms or features within the bluer region. There may be some minor disruption within the galaxy. Overall, the galaxy exhibits properties consistent with a disk galaxy.
