The galaxy presents as a disturbed system, likely undergoing a merger. A luminous central region is apparent, potentially indicative of an actively star-forming galactic nucleus or nuclei. Faint, diffuse spiral arm structures appear disturbed, with a distorted morphology suggesting tidal interactions with another galactic body. The disk is not clearly edge-on. The color gradient shifts from yellowish in the center to a bluer hue at the outer edges. There are no strong signs of a large bulge or a bar structure, suggesting it is not a well-defined spiral. A high merger fraction is likely. Overall, the object is an intermediate mass galaxy with suppressed star formation, and likely in the final stages of merging.
