The galaxy presents as a lenticular or early-type spiral morphology. It exhibits a smooth, centrally concentrated spheroid of stellar mass. A slight ellipticity is observed. The overall color suggests a moderately evolved stellar population, with a discernible but not prominent blue tinge indicating the presence of some ongoing star formation. There is no readily apparent dust lane or spiral arm structure. The galaxy shows no obvious signs of significant tidal interaction or recent merger events, appearing relatively undisturbed.
