The galaxy exhibits a generally smooth morphology, with a slightly elongated, elliptical shape. The central region displays a bright, concentrated luminosity, suggesting the presence of a significant galactic bulge. The light distribution diminishes gradually from the center towards the outer edges of the galaxy. There may be a weak disk structure, as hinted by a slight flattening and extended emission along a major axis. The galaxy's color appears yellowish-white, indicative of an older stellar population, with potentially some contribution from dust reddening. Overall, the image is consistent with a lenticular or early-type spiral galaxy.
