The galaxy presents as a single, fairly symmetrical object with a smooth, elliptical morphology. The color profile suggests a higher concentration of older stars, with a yellowish-white hue dominating the central region. There is a very subtle color gradient from the center outwards, transitioning to a slightly redder shade, particularly at what seem to be its periphery. The overall light distribution is fairly uniform, lacking any clear signs of spiral arms, dust lanes, or significant star-forming regions. Its structure appears undisturbed, with no obvious indications of ongoing or recent merger activity. It is well rounded in shape and shows no obvious sign of major disturbance or interaction with any other object.
