The galaxy presents a generally smooth appearance, with a centrally concentrated bulge. The overall shape is somewhere between round and elongated. There are no indications of strong tidal features or a major merger event. A subtle disk-like structure is suggested by the flattened shape, although distinct spiral arms or prominent dust lanes are absent. The galaxy displays a color gradient, appearing more yellow/orange in the central region. This color suggests an older stellar population dominating the bulge. A bluer hue extends outwards from the central region, indicative of some ongoing, though perhaps limited, star formation in the outer parts of the galaxy. Overall, this galaxy likely exhibits properties typical of a disk galaxy, that is likely quite massive with an intermediate star formation rate.
