The galaxy appears as a somewhat diffuse, centrally concentrated object. It exhibits a subtle elongation, potentially indicative of a disk-like structure, although no spiral arms are clearly resolved. The central region is brighter and appears to be more spheroidal.

There may be a minor perturbation or possible gravitational interaction occurring. It is not definitively merging, however there is the suggestion of some disturbed morphology, possibly in the form of a tidal feature.

The overall color of the galaxy suggests a mix of stellar populations. There is no evidence of a very young stellar population or prominent HII regions, as there is minimal blue coloring observed.
