The galaxy exhibits a spiral structure, though its arms appear somewhat indistinct and patchy. There's evidence of active star formation, particularly in the central regions and along some of the spiral arm segments, indicated by a bluer hue. The central bulge appears relatively moderate in size compared to the disk, with a yellowish color suggesting an older stellar population. There might be a faint bar feature running through the bulge. The spiral arms exhibit a relatively tight winding pattern. There's a possibility of minor disturbances or tidal features, which could suggest a recent interaction or merging event. There is a large central bright region, possibly due to star formation.
