The galaxy appears to be a spiral galaxy, oriented at an angle that is not quite face-on, but not fully edge-on either. The central bulge is moderately sized and exhibits a yellowish hue, indicative of an older stellar population. Two distinct, well-defined spiral arms extend from the central region, winding relatively tightly around the core of the galaxy. These arms are bluish in color, suggesting active star formation. There is no clear evidence of a bar structure within the galaxy. The disk appears somewhat disturbed, potentially indicating minor interactions or ongoing mergers. There is no evidence of major merging or tidal tails. The overall light distribution is uneven, with some regions appearing brighter and bluer than others, which could be due to variations in star formation rates across the galaxy.