The galaxy appears to be an elliptical type, characterized by a generally smooth and rounded morphology. There is a central, bright concentration of light suggesting a prominent galactic nucleus. The galaxy exhibits a slight elongation, deviating marginally from a perfect circular shape. Faint, diffuse features, potentially indicative of a disk or tidal disturbances, are only barely observed. The overall color profile suggests a relatively older stellar population, emitting primarily in the redder wavelengths, though there is a subtle presence of blue light in the extended disk. The galaxy does not show any obvious signs of a major ongoing merger, although some indications of minor interaction cannot be ruled out.
