The galaxy presents a largely smooth morphology, indicative of an elliptical or lenticular type. Its overall shape appears to be generally round. There is a lack of discernible spiral arm structure or significant dust lanes. The light distribution is centrally concentrated, with a gradual decrease in brightness outward from the core. There is no apparent ongoing major merger activity or significant tidal disturbance. The galaxy exhibits a relatively blue color, suggesting a population of relatively young stars.
