The galaxy presents as a relatively smooth, elliptical morphology with a bright, concentrated core.  A slight flattening is observed, tending towards an intermediate ellipticity. There's a discernible color gradient, with the central bulge exhibiting a yellowish-orange hue, potentially indicative of an older stellar population. The outer regions show a hint of bluer light, suggesting the presence of some younger stars, although the proportion appears low. The overall impression is of a galaxy that is not undergoing significant active star formation. There is no clear evidence of spiral arm structure or significant morphological disturbances from interactions or mergers.