The galaxy presents as an elliptical or lenticular structure, exhibiting a smooth, centrally concentrated luminosity profile. The core is bright and slightly elongated. Fainter, diffuse light extends outwards, with hints of some asymmetry. The color distribution appears to be uneven, with a generally redder hue overall but some faint hints of bluer regions near the periphery. There may be subtle signs of tidal distortion, particularly in the extensions of light that are not uniformly distributed around the central core. No prominent spiral arms or significant dust lanes are clearly visible. The galaxy appears relatively isolated, with no obvious signs of recent major mergers, though some minor interaction cannot be ruled out.
