The galaxy presents as a moderately luminous object with a somewhat elongated, elliptical morphology. The color profile suggests a dominant older stellar population, as indicated by the yellowish-red hue that permeates the central bulge. Fainter, bluer regions can be observed at the outer edges, indicative of younger star formation. The galaxy's overall structure appears relatively smooth, without any obvious signs of major disturbances or active merging events. There are some hints of a disk-like structure, but it is not clearly defined. The object's brightness gradually decreases from the core to the outer edges.
