The object presents as a merging system consisting of two distinct components. The primary component exhibits a relatively smooth morphology, with a concentrated central region and a diffuse halo. The color appears reddish, suggesting an older stellar population. The secondary component appears less defined, with a more irregular shape, indicating possible tidal disruption. A slight bluish tinge may indicate regions of recent star formation. There is a hint of a tidal tail or bridge of material connecting the two components, or a major disturbance within the galaxy, suggestive of gravitational interaction and likely an ongoing merger event. The system's overall shape is elliptical, with a slight elongation. No distinct spiral arms or bar structure are discernible.
