The galaxy presents a complex morphology, appearing to be in a late stage of interaction or merger. It is comprised of two distinct components.

The first, and perhaps originally dominant component, appears to be a relatively smooth, spheroidal structure. It exhibits a yellowish-white hue, suggesting an older stellar population with lower rates of ongoing star formation.

The second component is more diffuse, with a reddish-orange coloration indicative of dust obscuration and potentially recent star formation. It appears to be in the process of merging with the spheroidal component. The overall structure shows signs of tidal disruption, indicating a gravitationally disturbed system. There are noticeable asymmetries in the outer regions of the galaxy, likely the result of the ongoing merger. These tidal features indicate a dynamic system undergoing significant gravitational interactions.
