The galaxy presents as a lenticular, disk-shaped system, viewed at an oblique angle relative to its equatorial plane. The central bulge is bright and appears relatively smooth, suggesting an older stellar population. A faint disk is visible extending outwards from the bulge, with hints of spiral structure or possibly dust lanes. The color gradient suggests the presence of some ongoing star formation, particularly in the outer regions of the disk, though the redder overall color indicates a less active star formation rate. There are subtle signs of tidal disturbances, possibly indicative of past interactions or mergers. The system does not appear perfectly symmetrical, and the shape appears somewhat distorted. Overall, the morphology leans towards a transitioning state between a spiral and elliptical galaxy, with evidence of both ordered and disordered structures.
