The galaxy presents as a relatively smooth, centrally concentrated object. The morphology appears elliptical, with a high degree of roundness. The central region exhibits a bright, concentrated core that gradually fades into a more diffuse halo. There is little evidence of distinct spiral arms or significant star formation regions within the visible light spectrum. The outer regions appear smooth, and the galaxy appears to be relatively isolated, showing only minor signs of tidal interaction or disturbance. The galaxy's overall color suggests a population of older stars, with a relatively low ongoing star formation rate.
