The galaxy presents a distinct spiral structure, though somewhat tightly wound. The central bulge appears prominent and exhibits a yellowish hue, likely indicating an older stellar population. Fainter spiral arms extend outwards, displaying a bluish tint suggestive of ongoing star formation. Dust lanes are not clearly resolved, but there appears to be some obscuration along the spiral arms. The galaxy is observed at a moderate inclination. The overall shape seems to be elliptical. It is difficult to assess any merging or tidal features at this resolution.