The galaxy presents a predominantly smooth morphology, with minimal discernible substructure within its disk or halo. It appears somewhat elliptical, with a slight deviation from a perfectly circular shape. The central region exhibits a high surface brightness, suggesting a concentrated stellar population or an active galactic nucleus. A color gradient is observed, transitioning from a yellowish-white core to a reddish-hued outer region. This could indicate variations in stellar populations, with older, redder stars dominating the outskirts and younger, bluer stars concentrated towards the center. There are no apparent spiral arms, bars, or significant dust lanes visible in the image. The overall appearance suggests an evolved system, possibly an elliptical galaxy or a lenticular galaxy viewed at a moderate inclination angle. There is potentially some minor disturbances around the galaxy that could indicate there could be small tidal interactions or internal processes. The galaxy is relatively isolated in this field of view, with no immediately apparent companion galaxies or signs of a recent major merger.
