The galaxy presents as a centrally concentrated, yellowish-white object. Its shape is largely elliptical with a high degree of roundness, showing a lack of distinct spiral arm structures. The smooth appearance suggests a relatively evolved stellar population dominated by older stars. However, faint blue hues can also be detected in its outer regions. This indicates the presence of younger stars, suggesting some ongoing star formation. The overall color profile and morphology indicate that this galaxy is a late-type elliptical or an early-type spiral galaxy. The galaxy exhibits some signs of tidal disturbance suggesting a possible past interaction with another galaxy.
