The galaxy presents as a lenticular or edge-on spiral type. It exhibits a flattened, elongated morphology with a prominent central bulge. The bulge appears yellow-orange, suggesting an older stellar population with diminished star formation.  A faint disk is visible, oriented nearly edge-on, and is tinged with red. This implies a presence of dust obscuring the starlight. There is no indication of strong spiral arm structure. The galaxy appears relatively undisturbed, showing no signs of major mergers or significant tidal interactions.  The overall smoothness of the light distribution indicates a lack of recent major star-forming events, pointing to a relatively quiescent state.
