The galaxy exhibits a relatively smooth morphology, appearing as a somewhat diffuse, elliptical-like structure. Its color is predominantly yellow-red, suggesting a stellar population dominated by older stars. The light distribution is centrally concentrated, with a gradual decline in brightness toward the outer regions. There is no clear evidence of spiral arms or distinct features typically associated with younger, star-forming regions. No significant signs of tidal disturbances or ongoing merger activity are observed, though minor disturbances cannot be ruled out. The shape is generally rounded with a slight elongation, though it's difficult to ascertain the exact axis ratio given the image quality. Overall, the galaxy is likely an evolved system that has undergone significant star formation in the past.
