The galaxy presents as a moderately bright, elliptical-like structure with a smooth, diffuse morphology. The central region exhibits a high concentration of light, appearing almost uniformly luminous. The galaxy's color profile indicates a concentration of older stars, with a notable presence of reddish-yellow hues in the core, suggesting an evolved stellar population. Fainter, bluer extensions emanate from the central body indicating the possibility of ongoing, but low, star formation. There is no apparent strong dust lane or spiral arm structure. The overall shape is elongated, but without distinct or sharp features, suggesting a possible transition between elliptical and lenticular classification, with no signs of mergers or tidal disturbances observed.
