The galaxy displays a distinct spiral structure. The arms are tightly wound, originating from a central bulge region. These arms appear somewhat symmetrical, suggesting a relatively undisturbed morphology. Two dominant arms are observed, with evidence of branching and less defined segments that may indicate additional arm structures. The bulge is of moderate size relative to the overall galactic disk, and is a bright, concentrated region that blends smoothly into the spiral arms. There is no indication of a strong bar-like structure in the central region. The galaxy appears relatively isolated, with no major signs of ongoing mergers or significant tidal disturbances, although there might be some indications of minor interaction in the outer disk.
