The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated light profile with no discernable spiral arm structures or prominent dust lanes. The core exhibits a yellowish hue, suggesting a population of older stars. The halo appears more diffuse, with a subtle color gradient transitioning towards redder tones. There is no obvious tidal distortion or indications of a recent major merger event, though the morphology is slightly disturbed. The galaxy appears relatively isolated. The overall structure suggests an evolved system, possibly nearing the end of its star-forming lifecycle.
