The galaxy presents as a centrally concentrated, roughly elliptical form. Its color profile indicates a dominance of older stellar populations, with a yellowish-orange hue at the core, suggesting a lack of significant ongoing star formation in that region. The overall smoothness of the light distribution implies a lack of prominent spiral arms or other distinct structural features commonly associated with younger, disk-dominated galaxies. There's a subtle color gradient moving outward from the core, with the outer regions appearing slightly redder. This might indicate the presence of fainter, even older stars located further from the galactic center. The galaxy appears relatively undisturbed, showing no clear signs of recent major merger activity or tidal distortions. Based on these characteristics, this galaxy is consistent with an early-type, possibly elliptical, galaxy.
