The galaxy presents an elliptical morphology, exhibiting a smooth, concentrated light profile indicative of an early-type system. The core is relatively bright and diffuse, fading gradually into the outer regions. There are no apparent spiral arms, bars, or other distinct features commonly associated with disk galaxies. The galaxy appears largely undisturbed, showing no strong signs of tidal interactions or recent merger events. Its color suggests a population of older stars, with little evidence of active star formation.
