The galaxy presents as a diffuse object with no immediately discernible strong central bulge or distinct spiral arm structures. It is relatively compact. The galaxy's color profile appears varied, with a blend of redder and bluer regions indicating the presence of different stellar populations and/or dust obscuration. 

There appears to be some disturbed features, the structure suggests the possibility of a minor interaction or merging event. The galaxy exhibits irregular morphology that suggests the presence of tidal features or debris associated with a past interaction. It might also be that this shape is part of some imaging errors.
