The galaxy presents as a relatively compact, elliptical system. It exhibits a smooth, largely featureless morphology, with no discernible spiral arms or bar structures. The central region displays a concentrated luminosity, appearing brighter and more intensely colored, suggesting a higher density of stars or an active galactic nucleus. The overall color gradient transitions from a yellowish-white core to a slightly bluer halo, which could indicate a change in stellar populations. There appears to be no evidence of tidal distortions or ongoing mergers. The overall appearance is consistent with an early-type galaxy, likely an elliptical or lenticular galaxy, at a considerable distance.
