The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical morphology, tending towards circularity. The core displays a high surface brightness, with a gradual falloff in luminosity towards the outer regions. There is minimal discernible structure, such as spiral arms or a prominent bar. The galaxy appears largely undisturbed, lacking any obvious signs of ongoing or recent major merger events. The color profile suggests a population of older stars, as evidenced by the reddish-yellow hue, indicating a low rate of ongoing star formation. Faint irregularities in the outer regions may suggest minor gravitational interactions, but the dominant impression is that of a relaxed, evolved system.
