The galaxy presents as a relatively smooth, elongated structure. It exhibits a central, brighter region that appears nearly spheroidal, with a gradual decrease in luminosity towards the outer regions. Based on the color indices, the galaxy appears to be bluer in the central regions, suggesting the presence of a younger stellar population. There are no obvious spiral arm structures or significant dust lanes visible in the image. There is some slight peripheral asymmetry, possibly indicating a minor tidal disturbance or past interaction. Star formation appears low to moderate. Overall, this galaxy seems to be an elliptical galaxy with ongoing but relatively subdued star formation.
