The galaxy presents as a largely featureless elliptical or lenticular structure. Its morphology appears predominantly smooth and rounded, with a high degree of central concentration. The galaxy exhibits a noticeable color gradient, with the core appearing significantly yellower than the outer regions, which transition towards a bluer hue. This may indicate an older stellar population concentrated in the core, contrasted by younger stars in the surrounding areas. No significant spiral arms, bars, or tidal tails are discernible, suggesting minimal recent interaction or mergers. The galaxy's overall appearance is relatively undisturbed, pointing to a dynamically relaxed state. The redshift indicates the galaxy is at a considerable distance, which explains its small angular size.
