The galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology. It presents a spheroidal shape, with a high degree of roundness. The central region appears slightly brighter and more concentrated than the outer regions, with a gradual decrease in luminosity towards the edges, suggesting a high degree of symmetry. The color index suggests a stellar population that is relatively old and metal-rich. There is no apparent disk structure, spiral arms, or dust lanes. The galaxy does not appear to be undergoing any major mergers or tidal disturbances, though there may be some minor disturbances that are difficult to resolve. The lack of blue color suggests that there is relatively little star formation occurring within the galaxy. The galaxy's light is dominated by older, redder stars.
