The galaxy presents a predominantly smooth morphology, with a notable lack of distinct spiral arms or a well-defined disk structure. Its overall shape appears to be somewhat elongated but not highly so, trending towards a more elliptical form, though it has a relatively high degree of roundness. The galaxy exhibits a complex internal structure. There appears to be an active or recently completed merger event. Evidence points towards a ongoing or recent merger between the main galaxy and a smaller satellite galaxy. The system does show some minor disturbances in its outer regions which appear to be merger remnants. Overall, the galaxy exhibits a reddish-orange hue, indicating a population of older stars and potentially a lower rate of ongoing star formation.
