The galaxy appears as a centrally concentrated object with a generally smooth morphology. There is no strong evidence of spiral arm structure or a prominent disk component. The light profile suggests a relatively high degree of central concentration. The galaxy exhibits a slightly elliptical shape. The color gradient transitions from a yellowish-white core to a fainter, reddish-tinged outer region. The overall color suggests a population of older stars dominates, though there may be some ongoing, albeit subdued, star formation. There is a hint of minor disturbance, but overall it appears to be a relatively relaxed system.
