The galaxy presents as a largely smooth, elliptical structure. The central region exhibits a high concentration of light, appearing bright yellow. The luminosity gradually decreases toward the outer edges, which appear fainter and more diffuse. There is little evidence of distinct spiral arms or prominent dust lanes. The galaxy's shape is close to round, with a minimal elongation. There might be some evidence of minor disturbances in the outer regions of the galaxy, but they are subtle. The object does not appear to be actively merging with another galaxy. Overall, the morphology suggests a well-evolved system, consistent with an older stellar population.