The galaxy presents as a single, concentrated object with a generally smooth morphology. The light distribution indicates a centrally concentrated bulge or core, with a gradual falloff in intensity outwards. No distinct spiral arms or other obvious features such as bars or rings are discernible within the image. The overall shape appears roughly round, with only slight deviations from perfect circularity. The color profile shows a central region that appears slightly yellower, possibly indicating an older stellar population, with the outer regions showing hints of bluer hues, which may represent younger stars. There's no obvious sign of any major ongoing merger activity or strong tidal disturbances.
