The galaxy presents as a slightly elongated, disk-like structure with a smooth, centrally concentrated bulge. The overall color profile suggests a yellow-white hue, indicative of an older stellar population. There is a possible faint, disk-like component, though it is not sharply defined. Visual inspection of the galaxy suggests that the rate of star formation is relatively low. The general morphology of the galaxy does not suggest any ongoing major mergers or significant disturbances, though a subtle irregularity may be present in the faint, disk-like component. The size of the galaxy is moderate, neither particularly large nor unusually small.
