The galaxy presents a generally smooth, elliptical morphology. Its light profile is characterized by a high Sersic index, suggesting a centrally concentrated light distribution typical of spheroidal systems. The galaxy displays a slight elongation, with a relatively high axis ratio, indicating a departure from perfect circularity. 

The color gradients suggest an older stellar population dominates, with a redder central bulge and a gradual bluing towards the outer regions. There is no apparent evidence of prominent spiral arms or significant dust lanes. There may be some minor disturbances suggesting possible minor mergers.