The galaxy presents as a largely smooth, centrally concentrated object with a mostly elliptical morphology. The core exhibits a bright, yellowish hue. There is some asymmetry in the outer regions, but it primarily presents a rounded shape. The color suggests a population of older stars. There are no obvious spiral arm structures visible in the image. Evidence indicates it is a mature galaxy, and it does not show signs of an ongoing major merger. Subtle irregularities might suggest a past minor interaction.
