The galaxy presents a complex morphology, potentially indicative of an ongoing or recent interaction. The central region appears moderately smooth, with a subtle, elongated structure. The overall color of the galaxy is a relatively balanced mix of optical wavelengths. 

There are noticeable disturbances and asymmetries in the outer regions. A plume-like structure is visible, extending from the main body of the galaxy. This plume exhibits a bluer color than the central region, suggesting a population of younger, hotter stars. The asymmetry and the plume could indicate a tidal tail resulting from a gravitational interaction.

Given the color indices and apparent morphology, star formation appears to be present, at a reduced rate.
