The galaxy presents as a roughly elliptical object, with a smooth, diffuse appearance. The central region exhibits a brighter, more concentrated intensity, suggesting a higher density of stars or a possible active galactic nucleus. The outer regions appear to fade gradually, lacking distinct spiral arms or defined features. The overall color profile is dominated by warmer tones, with a yellowish core transitioning to a more reddish hue in the outer regions. There is little evidence of significant dust lanes or irregular structure. The galaxy appears relatively isolated, with no obvious signs of tidal interaction or ongoing merger events.
