The galaxy presents as an elongated, lenticular-like structure with a bright central bulge. Its disk is oriented nearly edge-on relative to our line of sight. The bulge exhibits a rounded morphology, and there is no obvious indication of boxiness. No significant dust lanes or distinct spiral arm structures are discernible from this perspective. The galaxy appears relatively smooth, with no major signs of recent or ongoing merging activity. There might be some minor disturbances. The galaxy possesses an intermediate mass. The color is a yellow-orange.
