The galaxy presents as a moderately luminous object, exhibiting a complex morphology indicative of an ongoing or recent merger event. The primary body of the galaxy appears relatively smooth, with a high concentration of light towards its center, suggesting a significant spheroidal component. This primary component has a yellow hue. There are two features to note: the red hue of the light indicates older stellar populations.

A distinct tidal tail or arm-like structure extends outward from the main body. The structure displays bluer colors, implying the presence of younger, hotter stars, potentially formed as a result of the interaction. The overall shape is more elongated. Given the features, it's possible that the galaxy is undergoing a minor or major merger.
