This galaxy appears to be an elliptical galaxy, characterized by its smooth, featureless morphology and round shape. The light distribution indicates a high degree of central concentration, with the luminosity decreasing gradually outwards from a bright core. There is a subtle color gradient, with the core exhibiting a yellowish-white hue, suggesting an older stellar population dominated by evolved stars. The outer regions appear slightly redder. The absence of spiral arms or a prominent disk suggests that this galaxy has undergone a period of relatively quiescent star formation history, though recent star formation may be present at a low level. There is no evidence of significant dust lanes or ongoing merger activity. The galaxy's overall appearance is consistent with a relaxed, evolved system.
