The galaxy presents an elliptical morphology, with an observed axis ratio indicating some degree of flattening. The light profile exhibits a concentrated core, surrounded by a more diffuse halo. Color gradients are apparent, with the core appearing yellower compared to the bluer outer regions. The Sersic index indicates the light profile is characteristic of an elliptical galaxy.  No spiral arm structures are discernible. There does not appear to be any signs of any major merging events occurring, though some disturbances cannot be completely ruled out given the image resolution. The size measurements, combined with the estimated redshift, suggest the galaxy is of intermediate physical extent.
