The galaxy presents as a moderately inclined, disk-like structure. It displays a relatively smooth appearance with a subtle central bulge. The overall color appears slightly redder, suggesting an older stellar population with a comparatively low rate of ongoing star formation. Some subtle distortions and irregularities are present, possibly indicative of minor gravitational interactions or internal disturbances. There is some evidence of faint tidal features or extended halos suggesting past merger events. The galaxy does not display any prominent spiral arm structure.
