The galaxy presents a largely smooth and concentrated appearance, with a central bulge that dominates its overall structure. It appears to be an elliptical galaxy, showing minimal disk-like features. There is an observed slight elongation and deviation from perfect roundness. No spiral arms or bar structures are discernible within the limitations of the image resolution. Faint blue tinges are barely visible around the central region. No indication of tidal tails or significant morphological disturbances are apparent, suggesting it is not undergoing a major merger. The overall color indices indicate the presence of an older stellar population, with a lesser presence of younger, bluer stars.
