The galaxy presents a largely smooth and elliptical morphology. The light distribution appears concentrated towards the center. The color profile suggests a dominant population of older stars, with a redder hue concentrated towards the galactic core that transitions to a slighty bluer hue towards the outer parts. There is no prominent disk structure, or spiral arm features visible. The round shape indicates it is likely an elliptical galaxy. There is no apparent evidence of a major ongoing merger or significant tidal disturbance. Overall, the galaxy appears to be a relatively undisturbed system, seemingly a massive elliptical galaxy composed of older stellar populations.
