The galaxy presents as a moderately luminous, relatively compact system. Its overall form appears to be elliptical, with a high degree of central concentration. The central region exhibits a yellowish-white hue, suggesting a population of older stars. The surrounding regions transition to a less intense, somewhat bluer color, hinting at the presence of some younger stars and potential ongoing, though subdued, star formation. There are no prominent spiral arms or bar structures visible. The overall structure is generally smooth, lacking significant morphological disturbances or signs of major interactions. Based on the color profile and morphology, this system is likely a relatively massive galaxy with a predominantly old stellar population, although some recent or ongoing star formation activity cannot be ruled out.
