The galaxy presents a generally smooth appearance, with a centrally concentrated bulge dominating its structure. The light profile appears relatively featureless, suggesting a lack of significant spiral arm structure or prominent dust lanes. There is a slight elongation, with an axis ratio that suggests it is not perfectly circular but rather somewhat elliptical in shape. The color is generally yellow, indicating an older stellar population, which may be indicative of a low star formation rate, or at least a star formation rate that is suppressed relative to its mass. There are faint indications of a more extended halo or disk component surrounding the central bulge, visible as a subtle change in color, becoming more blue. There is no immediately evident signs of ongoing mergers or major tidal disturbances. The overall impression is that of a relatively evolved galaxy dominated by an older stellar population.
