The galaxy appears as a single, relatively smooth object with a concentrated central region. It exhibits a generally elliptical morphology, appearing mostly round. The color profile suggests a population of older stars, evidenced by the yellow-red hue in the central bulge, indicating a lower rate of star formation in this region. The outer regions of the galaxy are fainter and somewhat bluer, suggesting the presence of younger stellar populations. There is no apparent strong spiral structure or significant dust lanes, though the limited resolution could obscure finer details. Overall, the galaxy presents as a mature, relatively undisturbed system.
