The galaxy presents as a smooth, elongated elliptical shape. The central region displays a concentrated luminosity gradient, appearing bright yellow-white. This suggests a higher density of older stellar populations within the core. The outer regions exhibit a gradual decrease in luminosity, with a subtle color shift towards a bluer hue. This could indicate a sparse population of younger, bluer stars within the galaxy's outer halo, or simply be a color gradient. There is no apparent spiral structure, dust lanes, or significant tidal features. The overall appearance is consistent with an early-type galaxy lacking significant ongoing star formation. Based on this, the stellar mass is likely very high. The galaxy appears relatively undisturbed, showing no signs of recent or ongoing major mergers.
