The galaxy presents as a centrally concentrated system with a smooth, elliptical morphology. A bright core region dominates the galaxy's light profile. A fainter, more diffuse halo surrounds the central region, exhibiting a slightly elongated shape. There's a subtle color gradient visible, with the central region appearing bluer, suggesting a possible presence of younger stellar populations or ongoing star formation activity. The outer regions show a redder hue, indicative of older, cooler stars. There is no clear evidence of spiral arms, bar structures, or significant dust lanes. Overall, the galaxy appears to be a relatively evolved system with a spheroidal shape.
