The galaxy presents as a spiral galaxy, exhibiting a well-defined disk structure viewed at an oblique angle. The central bulge is moderately prominent, appearing somewhat yellowish in color, suggesting an older stellar population. Two distinct spiral arms emanate from the bulge region, tightly wound around the galactic center. These arms showcase a bluish hue, indicative of ongoing star formation activity. The overall morphology suggests a galaxy where star formation is currently active but not exceptionally vigorous, with a possible bar feature. No signs of major disturbances due to mergers are readily apparent, though minor interactions can not be ruled out. The galaxy has moderate dust lanes, that break up the structure of the spiral arms.