This appears to be a spiral galaxy, viewed at a slight angle. The galaxy exhibits a prominent disk structure, although the angle makes it difficult to fully assess its shape. The presence of spiral arms is apparent, with a somewhat patchy and flocculent structure. Color variation exists across the galaxy, with a central, bright yellowish region likely indicating an older stellar population in the bulge. The outer regions of the disk display bluer colors, suggestive of ongoing star formation within the spiral arms. There's evidence of dust lanes within the disk, particularly near the center. The bulge appears to be moderately sized relative to the disk. There may be a bar present that is hard to see because of the angle. It is potentially undergoing some sort of interaction or merger.
