The galaxy presents as a somewhat disturbed spiral, with noticeable asymmetry in its structure. A prominent, though not dominant, bulge is observed, exhibiting a moderate concentration of light. One arm extends from the central region and appears distorted, possibly indicative of tidal interactions or ongoing merger activity. There is evidence of possible dust lanes or other obscuring material within the disk. A region of enhanced star formation, marked by a bluer color, is observable along a segment of the arm. The overall light profile is not particularly smooth, suggesting a galaxy that may be experiencing recent star formation or gravitational interactions. The spiral structure exhibits noticeable arms. The galaxy exhibits a bar-like structure across the center, with moderate strength.
