The galaxy presents as a somewhat elongated, cigar-shaped structure. The morphology suggests a galaxy undergoing some form of interaction or disturbance. There are no clear spiral arms. A significant portion of the galaxy's light is concentrated in a central bulge or core region that appears smooth. The outer regions show evidence of tidal features or distortions, such as tails or plumes, but the resolution limits detailed characterization. The color profile exhibits a gradient, with the central region appearing redder.
