The galaxy presents a generally smooth morphology with a subtle disc-like structure. It appears mostly spheroidal, though perhaps leaning more towards the "in-between" when assessed for roundness. The galaxy exhibits a color gradient; the central region is bright, transitioning toward a reddish-yellow hue, suggesting an older stellar population or significant dust obscuration. This contrasts with the bluer color observed in the outer disc or halo, indicative of younger stars or lower metallicity. There are no obvious signs of recent major mergers or tidal disturbances. The general luminosity profile indicates it is a massive galaxy with a significant population of stars, but a lower rate of star formation.
