The galaxy presents a distinct spiral morphology, viewed at an angle that is neither face-on nor edge-on. The spiral arms are well-defined, exhibiting a tightly wound structure, suggesting that the stars within the galaxy are being pulled inward. The central bulge is moderately prominent and displays a relatively smooth light distribution, indicating an older stellar population. The arms show a patchy distribution of light, possibly due to regions of active star formation. There are signs of minor disturbances in the outer disk, but no evidence of major ongoing merging activity. There may be a weak bar structure within the bulge. There appears to be two spiral arms present, but it is hard to count them.