The galaxy presents as a generally smooth, rounded object. The light distribution is centrally concentrated, exhibiting a bright yellowish core that fades gradually outwards into a diffuse, bluish halo. There is little evidence of spiral arm structure or dust lanes within the observed color bands. The overall morphology suggests an elliptical galaxy with a dominant spheroid component. Minor asymmetrical disturbances may be present in the outer regions, but the galaxy is not exhibiting any large-scale merging or major distortions of its shape. The color gradient, transitioning from yellowish in the core to bluish outwards, could indicate a radial variation in stellar populations, with a larger presence of younger, bluer stars in the outer halo.
