The galaxy presents a flattened, elliptical morphology. It is a relatively compact object, with a smooth, diffuse light profile. The core appears yellowish or slightly orange, potentially indicating an older stellar population. Fainter blue light extends from the central region, suggesting the presence of some younger stars or ongoing star formation within the galaxy's disk. A slight disturbance or asymmetry is noticed in the disk's structure. There might be a weak tidal feature or a minor interaction occurring, but overall the galaxy retains a fairly coherent structure.
