The galaxy presents as an elliptical morphology, exhibiting a smooth, featureless light distribution. The central region displays a concentrated brightness, suggesting a bulge component. The color gradient transitions from a yellowish-white core to a subtly bluer outer halo, which may indicate a difference in stellar populations or metallicity. The overall roundness of the galaxy is apparent, with no discernible disk or spiral arm structures. There is no clear evidence of tidal disturbances or ongoing merging activity.
