The galaxy presents as a relatively compact object, approximately round in appearance. The central region exhibits a brighter, more concentrated light distribution, suggesting a possible bulge. The overall color is slightly blue in the outer parts of the galaxy, potentially indicating recent or ongoing star formation within a disk-like structure. There appears to be some distortion or minor disturbances in the outer structure, potentially related to a previous minor interaction. The galaxy shows a somewhat smooth structure. No significant signs of a major merger are apparent, though a more in-depth analysis of the velocity field would be beneficial to confirm.
