The galaxy appears to be a spiral, viewed at an angle. A central bulge is visible, though not prominently defined, and a faint disk extends outwards. The disk itself seems smooth and lacks a notable degree of patchy or clumpy star formation. There is no evidence of a bar structure. The disk is slightly elongated in shape, with the overall form being somewhere between round and cigar-shaped. There's no clear sign of tidal tails or strong disturbances to indicate a recent major merger, though slight asymmetry within the disk could suggest a possible minor interaction or past disturbance. The galaxy's color gradient shows a bluer hue in the disk compared to the redder central bulge, which is indicative of a higher proportion of younger stars in the disk. The smooth appearance and color gradient suggest a spiral galaxy undergoing ongoing, but not necessarily intense, star formation.
