The galaxy presents as a roughly elliptical structure with a prominent central bulge. The core region exhibits a yellowish hue, suggesting an older stellar population. Extending outwards from the core, the galactic disc displays a bluer tint, potentially indicative of ongoing star formation. While some disk structure is evident, it appears somewhat disordered. There is a slight asymmetry observed in the outer regions, with hints of possible minor tidal disturbances or interactions. The overall morphology suggests a transition type between a pure elliptical and a spiral galaxy, perhaps an early-type spiral or a lenticular galaxy. Dust lanes are not clearly visible, but the overall structure appears relatively smooth.
