The galaxy exhibits a complex morphology, appearing to be undergoing a merger or strong interaction with another galaxy. There is a primary, somewhat spheroidal component with a dominant bluish hue, potentially indicating recent or ongoing star formation. Situated nearby is a secondary structure with a more diffuse, reddish appearance. This structure may be a tidally disrupted companion or a region of older stellar populations within the primary galaxy that has undergone tidal stripping. There are regions of visible disturbance. Dust lanes are not easily discernible, but the varied colors across the galaxy's body hints at differing levels of dust obscuration and stellar populations. The overall system size appears to be moderately extended, suggesting an intermediate-mass galaxy.
