The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. Its overall form is somewhat elongated, but not excessively so. The light distribution appears fairly uniform, lacking prominent spiral arms or distinct features suggesting active star formation regions. The color gradient shifts from a yellowish core, potentially indicating an older stellar population, to a bluer periphery, which might suggest the presence of younger stars. There are some hints of minor disturbances in the outer regions, although it is generally a well-defined object. The lack of prominent dust lanes or other significant morphological features points towards a galaxy that is nearing the end of its active star forming period. 
