The galaxy presents as an elliptical-like structure, with a smooth, diffuse light distribution. The core is notably brighter and exhibits a yellowish-white hue, suggesting a concentration of older stellar populations. Moving outward from the core, the light gradually decreases in intensity. A slight flattening of the galaxy's shape is observed. The overall color is a mix of yellow, green, and red tones, which could indicate a range of stellar ages and compositions. No distinct spiral arms or prominent dust lanes are discernible. The smoothness of the light profile suggests a lack of recent major mergers. There may be a minor disturbance noted in the light distribution, but it is not significant.
