The galaxy presents as a relatively smooth, elliptical-like structure. Its shape is mostly rounded. There is a concentration of light towards the center, with a gradual decrease in surface brightness moving outwards. Overall, the galaxy appears to be relatively undisturbed, lacking significant signs of tidal interactions or major mergers. The color suggests a population of older stars, indicated by the yellowish-red hue. There is no evidence of prominent spiral arms or dust lanes. Based on these observed characteristics, this is most likely an elliptical galaxy with high mass and old stars.
