The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The color gradient transitions from a yellowish-white core to a redder halo. There is no apparent spiral arm structure or evidence of significant dust lanes. The overall appearance suggests a mature stellar population with a high degree of spheroidal symmetry. The galaxy exhibits a moderate redshift, indicating a significant distance. There's a possible slight distortion in its shape, hinting at a potential weak gravitational interaction, but it's predominantly isolated in appearance. The galaxy's relatively small angular size suggests a moderate physical size, despite its considerable luminosity.
