The galaxy presents as a centrally concentrated object with a smooth, diffuse appearance. It exhibits a roughly elliptical morphology, appearing largely undisturbed. A subtle color gradient is observed, transitioning from a brighter, slightly bluer core to a fainter, redder outer region. No distinct spiral arms or prominent dust lanes are discernible. The overall light distribution suggests a relatively evolved stellar population, with possible ongoing, low-level star formation activity evidenced by the bluer core.
