The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated central bulge that dominates the overall light profile. There is a notable absence of spiral arm structures or dust lanes. The color gradient suggests an older stellar population, with a yellowish-orange hue concentrated in the core and a slightly bluer, albeit subdued, halo. The apparent roundness indicates a minimal degree of inclination relative to our line of sight. There is no obvious evidence of ongoing major mergers or significant tidal disturbances in the immediate vicinity of the galaxy. Faint wisps of light extend outwards, suggesting a diffuse galactic halo.