The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing largely rounded in shape. No prominent spiral arms or distinct disk structures are discernible. There are possible disturbances, however, with an extended faint halo. The primary body of the galaxy displays a color gradient from a bright, somewhat blue-white core to a slightly redder outer region. There is no evidence of a major ongoing merger. The object is likely a relatively massive system, with a moderate star formation rate.
