The galaxy presents as a single, somewhat diffuse object. The central region exhibits a higher surface brightness with a yellowish-orange hue, suggesting an older stellar population. This core gradually fades into a fainter, bluer halo. There is a possible disk structure. The overall light distribution suggests a relatively high stellar mass. The galaxy does not show obvious signs of active merging or major disturbances, although the overall symmetry is imperfect. The blue component implies ongoing, though likely modest, star formation within the galaxy's outer regions.
