The galaxy presents as a relatively smooth, elliptical morphology with a high degree of roundness. The central region exhibits a bright, concentrated luminosity, suggestive of a substantial galactic nucleus. Color gradients indicate a central concentration of older stellar populations, with a yellowish hue dominating the core. Moving outward, a subtle shift towards redder tones is observed, which may indicate the presence of an aging stellar population or dust obscuration in the outer regions. There's a subtle suggestion of very minor asymmetry in the outer envelope, though nothing suggestive of a major interaction or recent merger.
