This galaxy exhibits a complex morphology, appearing to be in a stage of interaction or recent merger. The primary component presents a relatively smooth, centrally concentrated bulge. There is evidence of disruption in the disk, with visible tidal features or arm fragments extending from the main body. These features indicate gravitational interaction with another galaxy. A secondary, smaller, and more irregular component is visible, showing possible tidal distortion from the larger primary. There is a hint of spiral arm structure in the primary component, though it's poorly defined. Dust lanes are subtle, suggesting a moderate level of ongoing star formation. The overall color of the galaxy indicates an older stellar population, predominantly yellow-red, with a small population of young blue stars.
