The galaxy presents as a somewhat elongated, lenticular structure. It appears moderately smooth, with a bright central bulge that diminishes in intensity toward the outer edges. The overall color gradient suggests a higher concentration of older stellar populations in the central region, giving it a more yellowish-red hue. Fainter, bluer regions appear interspersed throughout the galaxy, hinting at ongoing, but localized star formation. There is some indication of possible minor disturbances in the overall symmetry and shape, especially at the ends of the galaxy, but this is hard to verify due to the quality of the image. Its elliptical shape indicates a relatively high degree of internal ordering.
