The galaxy presents as a spiral type, displaying a prominent disk structure. There appears to be two distinct spiral arms. The arms exhibit a moderately wound morphology, indicative of intermediate shear. The arms are well-defined and extend noticeably from the central bulge. The bulge itself has a substantial amount of stars.

There is a slight asymmetry in the distribution of light within the disk, hinting at a possible minor interaction or internal disturbance. There does not seem to be a strong bar-like structure. There are no signs of major galactic merging. The core displays a concentrated brightness, suggestive of a central supermassive black hole that is not accreting or obscured by dust. The disk shows no signs of being edge-on. The galaxy exhibits a color gradient, with the central bulge appearing relatively redder compared to the bluer spiral arms.
