The galaxy presents as a dominant, elliptical morphology with a smooth light distribution. The central bulge appears bright and concentrated, exhibiting a yellowish hue, suggestive of an older stellar population. Fainter, diffuse emissions surround the central bulge, forming an extended halo. There is faint evidence of a disk structure, exhibiting blue-ish color, though it appears featureless and largely blended with the bulge and halo. The disk appears somewhat irregular in shape, with a hint of possible minor interaction, though it doesn't disrupt the general morphology. The galaxy is likely a massive system with suppressed star formation.
