The galaxy presents as a single, largely featureless object. It exhibits a slightly elliptical morphology. The light distribution appears relatively smooth, with a concentration of intensity towards the galactic center, gradually decreasing towards the periphery. There is no discernible spiral arm structure or dust lane features visible in the image. Minor disturbances may be present, but the galaxy does not exhibit a classical merging pattern. The apparent color is somewhat redder, indicative of an older stellar population, though blue light is still present. The galaxy appears to be neither perfectly round nor highly elongated.
