The galaxy presents as a single, yellowish-hued object with a relatively smooth appearance. There is a slight elongation to its morphology, though it tends toward being roundish. There is evidence of a possible interaction or recent merger event, as the structure appears slightly disturbed with a non-uniform surface brightness. Two distinct, brighter regions are observed, potentially indicating two core regions in the process of merging, or bright knots of star formation within the galaxy. The overall color suggests a population of older stars, and it's unlikely to be actively forming stars at a significant rate.
