The galaxy presents as a spiral type, although the angle of inclination complicates a definitive classification. There is a suggestion of spiral arm structure; however, the arms appear tightly wound and somewhat indistinct. A central bulge is discernible, exhibiting a moderate size relative to the overall galactic disk. The disk component appears dominant in terms of light distribution, with a blueish tinge suggestive of ongoing star formation. There is no obvious evidence of a strong bar feature. No signs of major mergers are observed, although the distorted morphology of the spiral arms could potentially indicate a minor interaction. The galactic nucleus is relatively bright and concentrated.