The galaxy presents as an elliptical morphology, exhibiting a smooth, nearly spherical distribution of light. There is a concentration of luminosity towards the central region, indicating a prominent galactic nucleus. The galaxy displays a color gradient, shifting from a pale yellow-white core to a slightly bluer periphery. This color variation suggests a potential difference in stellar populations, with older, redder stars dominating the core and younger, bluer stars residing in the outer regions. The absence of any visible spiral arms or significant dust lanes suggests a relatively undisturbed system, and the overall appearance aligns with that of a mature galaxy, potentially at a redshift of approximately 0.25. There appear to be no signs of ongoing mergers or interactions with other galaxies.
