The galaxy presents as a somewhat smooth, elongated structure, suggestive of a disk galaxy viewed at an oblique angle. There appears to be a central bulge, with a higher concentration of light, exhibiting a slightly yellowish color. The disk component extending from the bulge displays a bluer hue overall, potentially indicating regions of ongoing star formation. The galaxy does not appear to possess tightly wound spiral arms. Some visual irregularities within the disk suggest possible minor disturbances, perhaps resulting from a past interaction or internal dynamics. There is some indication of diffuse outer regions. The overall morphology leans toward a disk galaxy transitioning towards an elliptical form.
