This galaxy exhibits a roughly circular morphology with a bright, concentrated central bulge or core. There appears to be an extended, fainter halo surrounding the central region. The light distribution within the galaxy is not uniform, with some subtle irregularities or disturbances visible in the outer regions. The central region shows evidence of high activity, which is causing it to be more luminous than the outer regions. There is a potential indication of minor disturbance within the galactic halo, indicating that there might be possible minor interactions occurring. The light appears relatively smooth, and there is no clear indication of spiral arm structures.
