The galaxy exhibits a smooth, elliptical morphology with a high Sersic index. There is a noticeable central bulge, appearing as a bright, concentrated region. The galaxy shows a disk-like structure, although somewhat faint and obscured. The elongation is apparent, resulting in an axial ratio less than 1.0. There are no obvious signs of strong spiral arms or bar features. The overall color index suggests the presence of both old and young stellar populations, with the central region exhibiting a more yellow hue, potentially indicating older stars, and some greenish hints in the disk, which could be indicative of on-going star formation. The galaxy appears relatively isolated, showing no strong indications of interactions with other galaxies or major disturbances in its structure.
