The galaxy presents as a moderately bright, flattened elliptical or lenticular system. The central region exhibits a bright, concentrated core. Moving outward, the light smoothly decreases in intensity. The overall color profile suggests a dominant population of older stars, exhibiting a yellowish or reddish hue. The disk-like shape shows slight evidence of a possible faint, but subtle, outer disk, although it may simply be due to the distribution of light. There is no strong evidence of spiral arm structures. Minor irregularities might be visible, suggesting possible past interactions, but the overall structure is largely undisturbed. No prominent dust lanes are visible in this image.
