The galaxy presents as a fairly symmetric, elliptical-like structure with a smooth, diffuse light distribution. The central region exhibits a high concentration of light, appearing bright and yellowish, potentially indicating an older stellar population. There is a subtle color gradient, with the outer regions appearing slightly redder, suggesting a variation in stellar populations or dust content. No distinct spiral arms or prominent dust lanes are discernible, indicating a relatively featureless morphology. There is very little evidence of on-going star formation or other disturbance of this galaxy. The overall impression is of a quiescent galaxy, nearing the end of its life.
