The galaxy presents as a moderately luminous object with a distinct morphology suggesting an ongoing or recent interaction. The primary galaxy appears to be a disk galaxy, though its shape is not perfectly regular and presents a slight distortion. The central region exhibits a yellowish hue, potentially indicating an older stellar population.  A faint arm-like structure appears to extend from one side of the disk.

A second, smaller object is observed in close proximity. This object has a bluer color, suggesting it is composed of younger, hotter stars. Its morphology is irregular and somewhat diffuse. This secondary object is significantly less luminous. The proximity and irregular shape of the secondary object suggests a gravitational interaction. There is a moderate level of star formation occurring in the galaxy. The overall impression is of a system where one or more past or current gravitational interactions are likely influencing the morphological features observed.
