The galaxy presents a generally smooth morphology, suggesting an elliptical or lenticular type. The light distribution is concentrated towards the center, indicating a prominent galactic nucleus. The object exhibits a high degree of circularity, lacking any obvious signs of a disk structure or spiral arms. No major disturbances such as tidal tails or interacting companions are evident, implying relative isolation and gravitational stability. Faint color variations are present, with the central region exhibiting a more yellowish or redder hue, possibly indicative of an older stellar population, while the outer regions appear slightly bluer. The overall color is consistent with a galaxy dominated by older stars and relatively little ongoing star formation.
