The galaxy appears to be a relatively compact object. It exhibits a bright, concentrated central region which gradually diffuses outwards into a less defined halo. There are hints of some irregularities in the outer regions. The color profile seems to be a blend, with the core having a slightly bluer tint that transitions to more red in the surrounding halo. It does not appear to be a clear spiral or elliptical, possibly a more irregular structure. The overall morphology suggests a potential interaction or merger history, with some possible signs of disturbance in the shape. 
