The galaxy presents a predominantly disk-like morphology, observed face-on. A spiral structure is clearly visible, traced by regions of enhanced blue light, indicative of ongoing star formation. Two main spiral arms appear to dominate the galaxy's structure. The arms exhibit a moderate winding pattern, and can be seen trailing away from the relatively bright galactic bulge. The bulge is quite pronounced with a yellow/orange colour, suggesting an older stellar population. No significant bar structure is immediately apparent, but may be present. The galaxy shows no indication of any major merging event, although there might be evidence of minor tidal disturbances. Dust lanes may be present within the spiral arms, but are not very easily discernible. The overall appearance points towards a typical spiral galaxy with active star formation.