The galaxy presents as a largely smooth, elliptical-like structure. It exhibits a concentrated central bulge with a gradual fading of luminosity towards its outer edges. The color profile suggests a population of older stars, exhibiting a yellowish-white hue in the central regions. There is a subtle hint of a bluer component on what would be the bottom-right quadrant of the galaxy, potentially indicating a region with more active star formation. No distinct spiral arms or a prominent disk structure are discernible. The galaxy's overall morphology suggests it is relatively undisturbed, without obvious signs of recent major mergers or tidal interactions.
