The galaxy presents as a relatively smooth, centrally concentrated elliptical morphology. The light distribution appears largely uniform with no discernible spiral arm structures or significant dust lanes. The primary color is a yellowish hue suggesting an older stellar population, possibly dominated by evolved stars. The overall shape is nearly circular, with only a slight deviation toward an elliptical form. There may be slight evidence of tidal disturbances visible, with a potential minor asymmetry in its outer regions, but further investigation is required to confirm if this asymmetry is real or an artifact of the imaging process. The galaxy's light profile appears to gradually fade from a bright central core, outward toward the periphery.
