The galaxy presents as a relatively small, diffuse object. Its structure is largely amorphous, lacking a clear spiral or elliptical form. There is a hint of a disk-like structure, but it is subtle and potentially disturbed. The light profile appears somewhat irregular, suggesting possible tidal features or ongoing interactions. The galaxy's core region seems slightly brighter than the outer regions, however no significant bulge is present. Based on its red color, it is likely this is a galaxy with an older stellar population. The overall appearance points to a galaxy that may have experienced, or is currently experiencing, a merger or tidal interaction with another galaxy. There is no distinct arms or features to the disk. 
