The galaxy presents as a spiral structure with tightly wound arms emanating from a bright, concentrated central bulge. The spiral arms are well-defined and exhibit a clumpy morphology, suggesting regions of active star formation. The galaxy appears nearly face-on, allowing for a clear view of its overall structure. There is no evidence of a strong bar feature bisecting the bulge. The color profile indicates a relatively high presence of younger stellar populations throughout the spiral arms. The galaxy shows no signs of major disturbance or ongoing merging activity. The overall shape of the galaxy appears symmetrical and relatively undisturbed.
