The galaxy appears to be an elliptical galaxy with a smooth, mostly featureless morphology. It exhibits a centrally concentrated brightness profile, with a gradual decrease in luminosity outwards from the core. The galaxy is nearly round, showing minimal signs of significant disk-like structure or pronounced asymmetry. There is no evidence of ongoing major merging events or tidal disturbances. Color gradients are visible, with a central region that displays a slightly yellow-white hue, transitioning to a redder color in the outer regions. This color difference suggests a higher concentration of older, redder stellar populations towards the outer regions of the galaxy, with younger, bluer stars being less common.
