The galaxy presents a complex morphology, appearing disturbed, potentially indicative of an ongoing or recent interaction. The primary body exhibits an overall elongated shape, diverging from a perfectly elliptical form. There's an obvious indication of two distinct components, suggesting the possibility of a merger. One component displays a bluer hue, suggestive of more recent star formation or a younger stellar population. The other component exhibits a more yellow/red color, potentially indicating an older stellar population or a higher dust content attenuating blue light. A faint, extended structure seems to emanate from the main body. The galaxy does not display a clear disk-like structure; however, its shape would be best characterized as in between round and cigar-shaped.
