The galaxy appears as a relatively smooth, elliptical structure with a noticeable central concentration of light. Its overall shape is generally round, lacking any obvious disk-like features or strong asymmetries. The galaxy displays a color gradient, with the core region appearing more yellow or reddish, suggesting an older stellar population, while the outer regions appear slightly bluer, hinting at the presence of younger, hotter stars or a small amount of ongoing star formation. There are no prominent tidal tails, dust lanes, or other signs of recent major merger activity, indicating the galaxy is relatively undisturbed. The galaxy shows an apparent moderate redshift, which places it at a significant cosmological distance. Based on the colors, it has an intermediate mass compared to other galaxies. The light from this galaxy is consistent with a population of primarily older stars, as there is no sign of an active star forming region.
