This galaxy presents as a generally smooth and featureless object, with a somewhat elliptical morphology, elongated across its major axis. A bright, concentrated central bulge is present, which appears yellow-white in color, suggesting a population of older, cooler stars. The surrounding galactic disc exhibits a bluer hue, indicating the presence of younger, hotter stars and potentially ongoing star formation. There are subtle hints of spiral structure, although these features are not well-defined. The galaxy appears relatively isolated, without any obvious signs of major tidal disturbances or ongoing mergers, although there may be a minor distortion that suggests past gravitational interaction. The light from this galaxy has been redshifted, indicating that it is a considerable distance from our own.
