The galaxy appears to be a relatively smooth, centrally concentrated object. The light distribution suggests an elliptical morphology, with a high degree of central symmetry.  There is a slight elongation but overall, it appears quite round. No distinct spiral arms or bar structures are visible.  The color profile is somewhat uniform, with a suggestion of a slightly redder central region, which is consistent with an older stellar population. There is some sign of a merger or disturbance in the galaxy's light.
