The galaxy exhibits a complex morphology, indicative of an ongoing or recent interaction. A significant disturbance in the galactic structure is apparent.

The primary body of the galaxy presents an ill-defined shape, with a deviation from a regular elliptical or spiral form. There are areas of increased surface brightness suggestive of active star formation regions. The color gradients across the galaxy suggest variations in stellar populations.

Evidence points toward a possible merging event. There appears to be a tail like structure that extends from the core, further supporting the possibility of an interaction with another galactic body. The center of the galaxy presents a redder hue and a relatively smooth appearance which could be associated with an older stellar population within the galaxy.

Overall, this galaxy demonstrates characteristics of dynamical activity, likely induced by gravitational interactions with another galaxy. Further analysis may reveal if it is currently undergoing a merger or if it is a tidal stream remnant.
