The galaxy presents as a relatively smooth, concentrated object. Its central region appears bright and yellowish, indicating an older stellar population. The overall shape approximates an elliptical form, though some asymmetry is present. There's a hint of a diffuse outer halo, appearing fainter and bluer, suggesting the presence of some younger stars or potentially ongoing, though subdued, star formation activity at the periphery. No distinct spiral arms or bar structures are discernible. Minor disturbances seem to be present with some asymmetrical warping of the overall light distribution. The galaxy appears relatively isolated, lacking any obvious signs of recent major merger events.
