The galaxy appears to be a relatively compact and smooth system. It exhibits a somewhat elliptical morphology, although it is close to being round. There is a central concentration of light that gradually fades towards the outer regions, without any distinct spiral arm structures visible. There is a subtle blue tint, potentially indicating some ongoing star formation, but the galaxy generally lacks prominent features like dust lanes or bright knots associated with active star-forming regions. There is a suggestion of a slight disturbance in the galaxy’s form, though it is not merging with any other objects.
