The galaxy presents as a moderately bright, centrally concentrated object. Its overall morphology appears predominantly smooth, with a high degree of central concentration. The light distribution suggests a spheroid-like shape. There is a slight elongation in the vertical direction. The color gradient transitions smoothly from a bright, yellowish core to a redder, more diffuse outer region. Evidence of significant disk structures or spiral arms is absent. The outer regions show faint extensions indicating some low level star formation activity. There is no significant evidence of major tidal disturbances or ongoing merger activity.
