The galaxy presents as a generally smooth, elliptical-like structure. It exhibits a centrally concentrated brightness profile, with a bright, unresolved core that gradually fades into the surrounding halo. The galaxy's overall shape appears slightly elongated, departing somewhat from perfect circularity. There's no readily apparent evidence of significant spiral arm structure or major disturbances indicative of recent or ongoing mergers. Minor disturbances appear to be present. The colour profile suggests a relatively evolved stellar population, leaning towards redder wavelengths.
