The galaxy presents as a relatively compact object. Its overall morphology appears smooth and largely featureless, with a high degree of rotational symmetry. It appears nearly circular in projection, indicating a possible elliptical or lenticular classification. A faint central concentration of light is observed, surrounded by a more diffuse halo. The galaxy displays a subtle color gradient, appearing slightly bluer in its outer regions compared to the more yellow-orange hue of the core. This might imply ongoing, but relatively low levels of star formation in the outskirts. There are no prominent spiral arms, bar structures, or tidal tails visible in the image. The galaxy's apparent size is small, indicative of its great distance. No signs of recent major merger events are observed. The image is consistent with the galaxy being a passively evolving system.