The observed galaxy exhibits an edge-on disk morphology. A prominent, centrally concentrated bulge is visible, appearing somewhat rounded in shape. The disk appears relatively smooth, lacking obvious spiral arm structures or distinct features. Dust lane obscuration appears to be present, though subtle. The galaxy exhibits a redder hue, indicating an older stellar population and/or significant dust content. Overall, the galaxy appears to be a relatively undisturbed disk system with a noticeable bulge.
