This galaxy presents as a system of interacting components. The primary structure appears to be a relatively smooth, centrally concentrated body. Color gradients suggest a possible bulge component exhibiting older stellar populations. The overall morphology is somewhat elongated, leaning towards a prolate spheroid.

A secondary, smaller component is visible, separate from the main body. This component exhibits a bluer color, indicating younger stellar populations and potential ongoing star formation. A faint bridge or tidal feature is also weakly indicated and appears to connect the primary and secondary components, suggesting gravitational interaction. There are no obvious spiral arm structures present in either the primary or secondary components, though lower resolution makes such determination difficult. The system appears to be in a relatively advanced state of merging.
