This galaxy presents as a relatively smooth, centrally concentrated object, with some indication of a disk-like structure. The central bulge exhibits a yellowish-red hue, suggesting an older stellar population likely dominated by red giant stars. Surrounding the bulge, there's a bluer halo, potentially indicative of ongoing or recent star formation, though it does not appear particularly active. The overall shape leans slightly towards being rounded, rather than elongated or irregular, however, it is not perfectly round. There is a slight asymmetry in the outer regions, hinting at possible minor gravitational interactions or internal disturbances, but not on a large scale. Based on color and structure, the galaxy may be a disk galaxy of intermediate mass with moderate levels of star formation.
