The galaxy presents as a largely smooth, concentrated structure. The dominant feature is a bright, central bulge, exhibiting a yellowish-white hue, suggesting an older stellar population. A fainter, diffuse halo surrounds the bulge. The galaxy appears relatively circular in shape. There is a subtle indication of a faint disk component with bluer regions, hinting at the presence of some ongoing star formation within the disk, though this is not a dominant characteristic. There is a minor asymmetry in the outer regions, which could potentially indicate a past or minor interaction, but this is uncertain based on the image alone. The overall light profile is centrally concentrated, decreasing outwards from the core.
