The galaxy presents a generally smooth, elliptical morphology, with a high degree of roundness. The core region exhibits a strong concentration of light, appearing bright yellow, likely indicating a population of older stars. A subtle, less concentrated halo of bluish light surrounds the central region. This outer halo may suggest the presence of younger stars or regions of active star formation, although it is not strongly pronounced. There are no apparent signs of spiral arms, bars, or significant tidal disturbances, suggesting the galaxy is relatively undisturbed and potentially evolved. It is likely a relatively massive system, given its apparent size and luminosity, with a moderately low star formation rate. There is little evidence of significant dust lanes or other morphological features associated with ongoing mergers or interactions.
