The galaxy presents an elliptical morphology, although not perfectly spherical. It exhibits a smooth, somewhat diffuse appearance without prominent spiral arms or distinct features. The central region is noticeably brighter and more concentrated, suggesting a significant stellar population and/or possible active galactic nucleus. The color profile indicates a redder hue towards the center, transitioning to a slightly bluer tint in the outer regions. This could suggest the presence of older stellar populations in the core and relatively younger stars in the outskirts. There appears to be a very slight warping or tidal disturbance visible on one side of the galaxy, hinting at a potential past interaction with a smaller galaxy.
