The galaxy presents as a spiral structure. A prominent central bulge is observed, appearing moderately sized and luminous. Two distinct spiral arms emanate from the central bulge, winding moderately tightly around the galaxy. A strong bar feature is observed across the bulge. The disk appears face-on. There is no apparent evidence of any major merging activity or significant tidal disturbance. The color profile suggests an actively star-forming disk, with a relatively redder central bulge indicative of an older stellar population. The galaxy disk appears smooth and not clumpy.
