This galaxy presents as a moderately inclined, disk-shaped system. Its light is dominated by older stellar populations, suggesting relatively low ongoing star formation overall, with the bulk of star formation happening in the galaxy's center. The central bulge exhibits a smooth appearance, indicating a well-mixed stellar population, and it displays an elliptical shape, which may suggest this is a spiral galaxy. The galaxy appears to be generally undisturbed. Faint dust lanes are present, but not pronounced. Its faint blue colors, seen mostly on one side, are likely due to the formation of younger stars, and the redder colors around the center are likely due to older populations of stars.
