The galaxy appears to be a merging system, with at least two distinct nuclei visible. The overall color is reddish-orange, suggesting an older stellar population and significant dust content. The morphology is disturbed, lacking a clear spiral or elliptical structure, indicative of gravitational interactions. The galaxy exhibits a generally smooth appearance, with some evidence of tidal features or extended diffuse light surrounding the main body. Given the disturbed morphology, it is likely experiencing enhanced star formation activity, although it is not immediately apparent from the visual image.
