This galaxy exhibits a predominantly smooth morphology, appearing largely featureless. The light is concentrated towards the center. The object presents as moderately round, with only a slight deviation from a perfectly circular shape. There is no clear evidence of major disturbances or ongoing merging events. The overall color is trending towards redder wavelengths, implying an older stellar population and a reduced rate of star formation. Based on the red-shifted color, the galaxy seems to be a substantial distance from our own.
