The galaxy presents an intermediate morphology between smooth and featured. Approximately 56% of the light appears smooth, while 37% shows distinct features or a disk-like structure. The overall shape is somewhat elongated. The central region exhibits a yellow hue, suggesting an older stellar population, potentially a bulge. Fainter, bluer regions are visible extending outwards from the central body of the galaxy. This suggests the possibility of ongoing or recent star formation. There appears to be some type of tidal interaction or merger event happening, indicated by disturbances in the galaxy's overall shape and structure. These disturbances include a faint but noticeable tail or bridge of material extending to one side of the galaxy.
