The galaxy presents as a relatively compact, elliptical-like object. Its light is dominated by a yellow-red hue, suggestive of an older stellar population. The galaxy has a smooth, symmetrical appearance with no discernable spiral arm structures or significant dust lanes. Its overall form appears largely undisturbed, exhibiting no obvious signs of ongoing major mergers or tidal interactions, but small disturbances cannot be ruled out. The concentration of light is high in the central region, gradually decreasing outwards.
