The galaxy appears to be a relatively smooth, elliptical-like structure. Its core exhibits a bright yellowish-orange hue, suggesting an older stellar population. There is a subtle color gradient towards the outer regions, with a slight shift towards redder tones. The overall form lacks any discernible spiral arms or significant dust lanes. It seems largely undisturbed, without major signs of ongoing mergers or tidal interactions. The light distribution indicates a centrally concentrated luminosity profile, characteristic of elliptical galaxies. Its morphology suggests it may be classified as an early-type galaxy.
