The galaxy presents a generally smooth appearance with a notable central bulge. The light distribution suggests a significant concentration of older stars, which contribute to the overall yellowish hue. There's a subtle extension of light around the central region, hinting at a disk component, though it's not sharply defined. It is slightly elongated in shape, deviating from a perfect circular symmetry. Indications of possible minor disturbances or interactions are subtle, though the overall structure appears largely undisturbed. The color profile indicates moderate star formation.
