The galaxy presents as a largely smooth, elliptical-like structure. The light distribution appears centrally concentrated with a gradual decrease in surface brightness outward from the core. Color gradients are subtle but present; the central region exhibits a yellowish to reddish hue, potentially indicating an older stellar population and/or dust obscuration. Moving outwards, the color shifts slightly towards bluer shades, possibly signifying the presence of younger stars, although this is less prominent. The galaxy appears relatively undisturbed, with no readily apparent signs of major mergers or tidal features. There is a slight asymmetry in the isophotes, suggestive of a minor interaction or perhaps an internal dust lane. Overall, the galaxy's morphology suggests a evolved system with a moderate stellar mass and a low rate of current star formation.
