The galaxy presents as a lenticular or possibly an edge-on spiral system. It exhibits a pronounced central bulge, appearing smooth and concentrated. There's a faint disk component that extends along a primary axis, appearing elongated. Color gradients are subtle, but indicate that the bulge is relatively redder compared to the disk, suggesting an older stellar population. The disk appears to be subtly bluer, which could indicate recent star formation. The overall morphology appears relatively undisturbed, and there is no clear visual evidence of a major ongoing merger event, though the galaxy's elongated shape suggests a minor tidal interaction cannot be ruled out. Given the system's redder color, smooth profile and lack of resolved spiral arms, it is likely to be undergoing passive evolution with a very low rate of star formation.
