The galaxy presents a relatively smooth and concentrated light profile, appearing elliptical in shape. The core exhibits a bright, yellowish hue, suggesting an older stellar population dominating the central region. There is a gradual decrease in luminosity moving outward from the core, with a faint, diffuse halo that blends into the background. While the overall structure appears largely undisturbed, there is a subtle asymmetry in the outer regions, potentially indicative of a minor interaction or past merger event. The galaxy displays a moderate redshift, placing it at a considerable cosmological distance. The relative blueness of the light suggests there may still be some active star formation within the galaxy, although dominated by the yellow and red light from older stars.
