The galaxy presents as a somewhat elliptical, though not perfectly spherical, system. The light is concentrated towards the center, which exhibits a bright, yellowish hue suggestive of an older stellar population. Moving outward from the center, a diffuse, greenish-tinted region is visible. This region has some blotches and distortions, possibly indicating minor disturbances or uneven distribution of interstellar material. There appears to be little evidence of distinct spiral arm structures. The overall form hints at a potentially merging system, with a primary body that has begun to settle into an elliptical shape.