The galaxy exhibits a largely elliptical morphology with a smooth profile and a relatively high Sersic index, suggesting a dominant bulge component. The concentration of light is high in the central region, decreasing gradually towards the outer edges. Color gradients are subtle, with a slightly bluer hue in the inner regions compared to the periphery, potentially indicating ongoing, low-level star formation closer to the core. The galaxy appears undisturbed, with no signs of tidal features, major mergers, or significant disk structures. The overall shape suggests a relaxed system.
