The galaxy presents as a luminous, relatively smooth structure. Its overall morphology appears elliptical, with the light distribution concentrated towards a bright, moderately defined core. The color profile suggests a population of older stars dominating the light output, exhibiting a yellowish hue. There is little evidence of spiral arms or significant dust lanes; the galaxy appears primarily spheroidal in shape. A fainter object appears in the foreground, which may or may not be related. The galaxy exhibits characteristics consistent with a relatively low rate of star formation. The overall appearance suggests a galaxy that has undergone significant evolution and may be approaching a quiescent state.
