The galaxy presents a somewhat elliptical morphology. Its overall color suggests a significant population of older stars, with a dominant yellowish-red hue. The light distribution appears relatively smooth and centralized, showing limited or no distinct spiral arm structure. There is a slight disturbance visible as an irregular extension of the galactic halo to the left side of the galactic center. The galaxy seems to have a relatively compact central bulge, with a gradual decrease in luminosity towards the outer regions. The galaxy appears to be fairly isolated, with no obvious signs of interactions with nearby galaxies. The overall impression is that of a relatively massive galaxy undergoing little active star formation.
