The galaxy presents as an elliptical system with a smooth, diffuse morphology. There is a noticeable concentration of light towards the galactic center. The galaxy exhibits a color gradient, transitioning from a redder core to a slightly bluer halo. This may be due to a differential in stellar populations, with older, redder stars concentrated in the core, and younger, bluer stars populating the outskirts. The overall shape appears somewhat elongated, indicating a possible deviation from a perfectly spherical structure. There are no obvious signs of significant tidal disturbances or ongoing mergers, suggesting the galaxy is relatively undisturbed. The light is relatively evenly distributed, implying a fairly homogeneous distribution of stars throughout the galaxy.
