The galaxy presents as a relatively compact structure with a noticeable central bulge, suggesting a considerable spheroidal component. Its overall shape is generally round. The color profile indicates the presence of both older stellar populations, contributing to the redder hues, and regions of ongoing star formation, evident in the bluer tints. There appears to be some level of disturbance within the galaxy, perhaps indicative of minor interactions or internal dynamical processes. While the majority of the galaxy appears smooth, there might be a faint indication of a disk-like structure, or some form of spiral arm feature.
