The galaxy presents as a somewhat edge-on spiral or lenticular galaxy. A prominent dust lane bisects the galaxy, obscuring a significant portion of the central bulge. The bulge appears relatively small and has a smooth profile. Star formation appears most active in the disk, particularly in a few localized regions. Overall, the light distribution within the galaxy is somewhat uneven, with the disk appearing brighter on one side. The galaxy exhibits a slight blue tint and a noticeable redder bulge. The inclination angle obscures the details, but the visible morphology suggests a well-defined disk structure.
