The galaxy presents as a moderately bright, elongated elliptical. A concentration of yellow light is observed towards the galactic center, surrounded by a more diffuse, lower surface brightness halo. The lack of spiral arm structure, combined with its elliptical shape, suggests a relatively evolved system, where much of the gas and dust has been consumed in star formation or expelled from the galaxy. The smooth light distribution further supports the absence of recent major merger events. The color profile indicates a population of older stars, with a redder hue dominating the central bulge, transitioning to slightly bluer tones in the outer regions, likely due to a small population of younger stars. The overall morphology appears undisturbed, with no significant tidal features or asymmetries detected, thus it is a very stable system.
