The galaxy exhibits a generally smooth morphology, with a concentrated central bulge. The light distribution transitions from a bright, yellowish core to a more diffuse, greenish outer region. While appearing mostly featureless at this resolution, there may be hints of a slightly flattened or elliptical shape rather than perfectly circular symmetry. No distinct spiral arm structures or signs of major disturbances are evident. The color gradient suggests a potentially older stellar population dominating the central region, with perhaps some ongoing star formation in the outer regions, although this is not definitively discernible from the image.
