The galaxy appears to be a relatively compact object, exhibiting a roughly elliptical shape with a bright, concentrated central region. There is a subtle asymmetry in the outer regions of the galaxy. While a diffuse, blue-ish halo surrounds the core, the halo appears slightly more elongated on one side, suggesting a potential disturbance or interaction. There appears to be some subtle hints of tidal features. The central region shows no signs of spiral arm structure. The color distribution suggests the presence of both older, redder stellar populations in the core and bluer, possibly younger populations within the outer halo. Overall, the galaxy may be experiencing, or have recently experienced, some form of gravitational interaction or disturbance that has affected its morphology.
