The galaxy presents a spiral morphology, with a relatively smooth central bulge. Its color suggests a population of aging stars in this region, likely with a small population of dust and gas. The spiral arms are well-defined, exhibiting a patchy distribution of bluer regions indicative of ongoing star formation. These regions are concentrated along the arms, suggesting the presence of HII regions or young star clusters. There appears to be a disturbance within the spiral structure that may be the sign of a minor merger event. The overall structure indicates a galaxy that has undergone significant evolution, with evidence of both past and present star formation activity.
