This galaxy presents as a somewhat elliptical, disk-like structure. It exhibits a central bulge that is bright and concentrated. The overall color appears to be yellowish-red, suggesting a population of older stars and a diminished rate of ongoing star formation. There is little evidence of prominent spiral arms or significant dust lanes. The galaxy’s morphology indicates it is likely an intermediate type, possibly transitioning from a spiral to an elliptical form. There are no obvious signs of a major ongoing merger, though some minor disturbances cannot be ruled out based on this single image. The galaxy's shape is largely "in between", neither distinctly round nor cigar-shaped. The galaxy shows a smooth appearance overall, suggesting it is likely in a late stage of evolution.
