The galaxy presents as a roughly elliptical structure, though not perfectly circular. There is a slightly elongated morphology, with a color gradient noticeable across the galaxy’s extent. The central region appears brighter and exhibits a yellowish-white hue, suggesting a concentration of older stellar populations. Moving outwards from the core, the color shifts toward a bluer tone in the outer regions, which may indicate the presence of younger, hotter stars. There is no distinct spiral arm structure visible, nor is there a prominent central bulge that would classify it as a pure elliptical. A minor asymmetry is hinted at, perhaps due to a past interaction. Overall, the galaxy seems to be in a relatively quiescent state, though with some evidence of ongoing or recent star formation in its outer reaches.
