This galaxy exhibits a disk-like structure viewed at an oblique angle, nearing edge-on. A distinct central bulge, concentrated and yellowish-white in color, is visible. Extending from this bulge are faint, bluish-white spiral arms, though they lack well-defined structure and are somewhat diffuse. 

A prominent tidal tail or plume emanates from the main body of the galaxy. It appears elongated and diffuse, with a bluer color suggesting the presence of young, hot stars or ionized gas. This feature indicates possible gravitational interaction or a past merger event.

The galaxy's overall morphology suggests it is undergoing or has recently experienced significant disturbance, with substantial disruption in its spiral arm structure and the presence of the tidal tail.
