The galaxy presents an irregular morphology. It exhibits a disturbed structure, indicating a possible ongoing or recent interaction or merger event. The primary body appears diffuse and somewhat elongated. A distinct, brighter region is seen to the south, possibly a tidal tail or a separate merging galaxy. There is a noticeable asymmetry in the light distribution, suggesting a non-equilibrium state. Star formation appears to be occurring at a relatively low rate. The galaxy’s overall color suggests a moderate population of older stars with some younger, bluer stars present within the disturbed features.
