The galaxy presents as a generally smooth, elliptical-like morphology, exhibiting a concentrated central bulge and a diffuse halo. The galaxy displays a yellow-orange hue in its central region, possibly indicative of an older stellar population or significant dust content absorbing blue light. The outer regions of the galaxy appear slightly greener, which could be indicative of some star formation. The overall roundness of the galaxy suggests a minimal degree of disk-like structure. There is no significant evidence of tidal disturbances or interaction with other galaxies in this image, implying it is relatively undisturbed.
