The galaxy presents as a single, relatively smooth concentration of light. Its morphology is predominantly elliptical, exhibiting a high degree of roundness. There is a distinct central bulge that transitions gradually to a more diffuse halo. The color profile suggests an older stellar population, with a yellowish-red hue concentrated in the core that fades toward the edges. There's little evidence of spiral arms or disk-like features, and no indications of ongoing major mergers or tidal disturbances. The galaxy appears fairly isolated and undisturbed.
