The galaxy presents as a single, dominant object with a relatively smooth and rounded morphology. It lacks any discernible spiral arms or bar structures. The light profile appears centrally concentrated with a bright, somewhat diffused core. There is a gradual falloff in luminosity from the center outwards, forming a more elliptical shape with slightly more luminosity along the x-axis. The color index suggests a more evolved stellar population; this is indicated by a yellowish-red hue toward the galactic center. It appears undisturbed with no evidence of tidal tails or ongoing mergers. The red shift indicates that this galaxy is distant, with an inferred size of approximately 6 kpc.
