The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears elliptical or lenticular, lacking prominent spiral arms or a well-defined disk structure. The galaxy exhibits a radial color gradient, transitioning from a yellowish-white core to a bluer, more diffuse outer region. There is no apparent central bar. The galaxy’s overall structure suggests a system dominated by older stellar populations, but the bluer outskirts hint at ongoing, albeit modest, star formation activity. There is no evidence of any major mergers or tidal disturbances. The galaxy is largely undisturbed.