The galaxy appears as a centrally concentrated, luminous object with a smooth, elliptical morphology. There are no distinct spiral arms or bar structures visible in the image. The galaxy's light is dominated by yellow-white hues, suggesting a stellar population with a significant fraction of older stars. The overall structure exhibits a high degree of radial symmetry, with no obvious signs of tidal disturbances or recent merger activity in this image. The galaxy appears relatively isolated in the observed field. There is no dust visible.
