The galaxy presents as a relatively small, disk-shaped object. It exhibits a flattened spheroidal central bulge. The color distribution within the galaxy is complex; the bulge appears to be composed of an unknown object exhibiting red and magenta spectral signatures, surrounded by an area of cyan and yellow spectral signatures. An area of green extends outwards from this core. The outer regions are fainter, with a more diffuse light distribution. The galaxy appears to be relatively isolated with no immediately apparent companion galaxies or signs of recent major mergers. However, based on the slight asymmetry of the outer halo, there are possible minor tidal disturbances. Given the size of the galaxy and smooth light profile, this galaxy is most likely an elliptical galaxy with no disk component. The bright emission near the bulge of the galaxy might indicate active galactic nuclei activity or star formation. Further spectroscopic investigation is necessary to determine the redshift, and the nature of the central object, as well as the source of the green light.
