The galaxy exhibits a disturbed morphology, potentially indicating an ongoing or recent interaction. The light distribution is not uniform; it appears clumpy and asymmetric with multiple bright knots of light scattered throughout. These could be areas of enhanced star formation or remnants of tidal features. There is no clear evidence of a well-defined spiral structure or a dominant elliptical form. The general color of the galaxy appears to be reddish-orange, suggesting a population of older stars and a lack of significant ongoing star formation. However, the presence of the brighter, bluer knots indicates that there is still some active star formation present, albeit perhaps at a low rate.
