The galaxy presents a distinct spiral structure, appearing with two prominent, well-defined arms. The arms exhibit a medium winding, neither tightly coiled nor completely unwound. These arms emanate from a central bulge, which appears moderately sized relative to the overall galactic disk. A strong bar feature is visually apparent, bisecting the central bulge and likely influencing the arm structure. Within the spiral arms, hints of active star formation are suggested by subtle color variations and clumpy regions. The galaxy is observed nearly face-on, allowing for clear examination of its spiral morphology. There is no significant visual evidence of ongoing major mergers or strong tidal disturbances, however, some very subtle disturbances cannot be ruled out.
