The observed galaxy presents as an edge-on spiral, exhibiting a lenticular morphology. It displays a prominent central bulge, appearing somewhat rounded and concentrated. There is indication of a disk structure, although its features are largely obscured due to the edge-on viewing angle. The galaxy appears to be relatively undisturbed, with no significant signs of ongoing mergers or major tidal interactions, though a small, local disturbance is possible. The distribution of light suggests a moderate level of star formation.
