The galaxy presents as a centrally concentrated, relatively smooth object with a generally elliptical morphology. A bright, yellowish core dominates the galaxy's appearance, suggesting a significant population of older stars within the bulge. The surrounding halo exhibits a more diffuse light, with some hints of bluer regions. These hints could indicate regions of active star formation, although this is not definitively discernible from the available imagery. There is no evidence of strong spiral arms or a well-defined disk structure. Subtle color variations are present, with reddish hues in the lower regions, possibly indicating dust lanes or a different stellar population. Overall, the galaxy appears to be relatively undisturbed, lacking strong evidence of major merger events or tidal distortions.