The galaxy exhibits a generally smooth morphology with a highly concentrated central bulge that emits strongly in the g, r, and z bands, indicating the presence of an older stellar population. The central region appears nearly spherical. The outer regions of the galaxy display a less concentrated distribution of light, with some subtle evidence of a faint, diffuse disk structure. There is no apparent spiral structure or bar, and no indications of ongoing major mergers or significant tidal disturbances are visible. The color gradients suggest the presence of some star formation occurring, with slightly bluer regions present in the disk as compared to the core. Based on the roundness and smoothness, this is likely an elliptical galaxy. The galaxy appears to be relatively isolated, showing no signs of close companions or interactions that might affect its morphology.
