The galaxy presents as a somewhat diffuse, centrally concentrated object. The core region exhibits a yellow-white hue, suggesting an older stellar population. Moving outward, the color shifts to a cooler blue, hinting at the presence of younger, bluer stars in the outer regions. While no spiral arm structure is clearly discernible, there is some indication of a disk-like morphology. The galaxy appears to be relatively isolated, with minimal signs of tidal interactions or recent mergers, although the galaxy's structure is slightly disturbed. There are indications of minor disturbances but no signs of any ongoing significant mergers. Overall, the galaxy appears to be a relatively massive system undergoing moderate star formation.
