The observed galaxy presents as a smooth, elliptical structure. It exhibits a concentrated central bulge that appears a yellow-orange hue, indicative of an older stellar population. The galaxy displays a relatively gradual decline in luminosity from its center outwards. There is a subtle suggestion of a flattened disk-like shape, as the galaxy's profile is more elongated than perfectly circular. Faint wisps of bluer light can be seen along the periphery of the galaxy, which may indicate some ongoing, though limited, star formation activity. No significant tidal disturbances or signs of ongoing merger activity are evident. The galaxy appears relatively undisturbed.
