The galaxy presents a generally smooth morphology, exhibiting a concentrated central bulge that appears largely spheroidal in shape. There is a subtle elongation visible, suggesting a deviation from a perfectly circular form. The primary color component is a strong yellowish-orange hue, which may indicate a population of older stars. There is no immediately apparent spiral arm structure, and the overall texture appears relatively uniform, with no signs of major disturbances such as tidal tails or strong asymmetries. The faint presence of disk-like features cannot be ruled out, although these are subtle. Faint hint of blue color may suggest presence of younger stars. There may be some evidence of minor disturbances in the galaxy's overall form.
