The galaxy presents a largely smooth morphology with an elliptical shape. The central region exhibits a high concentration of light, appearing bright and yellowish. A faint, bluish extension is observed on one side, which suggests a possible tidal feature or minor disturbance. Overall, the galaxy appears relatively isolated and does not show strong evidence of a major ongoing merger, though some minor interaction cannot be ruled out based on the subtle asymmetry. The light distribution indicates a evolved stellar population.
