The galaxy presents as a predominantly smooth structure, with an ellipsoidal morphology. Its light profile appears fairly concentrated towards the center, exhibiting a gradual decrease in luminosity outward. There is a subtle color gradient across the galaxy, transitioning from a slightly bluer hue in the central regions to redder colors in the outer edges. This suggests a possible radial variation in stellar population or dust content. Some minor asymmetries or subtle features are visible that indicate there may have been some tidal interactions in the past, but no major merger is apparent. Overall, the galaxy appears to be a relatively evolved system, consistent with an elliptical or lenticular classification, and is in a relatively quiescent state of star formation.
