The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated central bulge that transitions smoothly into a more diffuse halo. The light profile is dominated by yellow and red hues, suggestive of an older stellar population with relatively little ongoing star formation. There is no visible evidence of spiral arms or a disk-like structure. The overall appearance is consistent with a massive, evolved galaxy, potentially an elliptical. The roundness of the galaxy suggests that it's relatively undisturbed. There is no discernible evidence of merging activity or significant tidal interactions in the image.
