This galaxy presents as a somewhat elongated, disk-like structure, viewed at an oblique angle, potentially nearly edge-on. It exhibits a relatively smooth appearance, with a concentrated central bulge region. Faint blue-ish halos extend from the central region, indicating areas of possible ongoing or recent star formation. There is a hint of asymmetry in the outer regions of the disk, but no major disturbances are observed, suggesting it is not currently undergoing a major merger event. It is possible this galaxy is a spiral galaxy, but the angle does not allow for clear observation of spiral arms. Overall, the galaxy appears to be relatively quiescent in terms of star formation activity.
