The galaxy presents as an edge-on spiral, exhibiting a distinct disk morphology. A pronounced bulge dominates the central region, appearing largely smooth with a slight boxy shape. The disk appears relatively thin and elongated. The central region appears reddish, likely indicating an older stellar population, while the outer edges of the disk show greenish hues, suggestive of ongoing star formation. There are no obvious signs of tidal disruption or significant merging activity, although some minor disturbance of the disk cannot be entirely ruled out.
