The galaxy presents as a primarily smooth, elliptical-like structure. There is a concentration of yellow-white light towards the center, indicating an older stellar population concentrated in the bulge region. Extending outward from this central region is a fainter, more diffuse halo of light. There is a subtle hint of bluer tones in this outer region, possibly suggesting some level of ongoing star formation, albeit at a low rate. The overall morphology appears relatively undisturbed with no signs of significant tidal features or ongoing major merger activity. Any presence of a disk component is not readily apparent from the image data. There is a chance that a minor disturbance may be slightly affecting the morphology, but any evidence of such a disturbance is not clear in the image.
