The galaxy presents as a largely smooth, elliptical-like structure with a high degree of central concentration. The color profile suggests an older stellar population dominating the core, exhibiting a yellowish-red hue, indicative of relatively low star formation. Fainter, somewhat bluer, diffuse light is observed in the outer regions of the galaxy, hinting at more recent, albeit subdued, star formation activity. The galaxy appears relatively undisturbed with no signs of major mergers or tidal interactions; subtle asymmetries, if present, are minimal. It displays a generally rounded morphology, showing minimal elongation or disk-like features.
