The galaxy presents a largely smooth morphology, exhibiting a concentrated central bulge with a more diffuse surrounding halo. The overall color profile suggests a relatively evolved stellar population, displaying a yellowish-orange hue concentrated in the core, indicative of older stars and a lack of significant ongoing star formation. The shape is generally elliptical, deviating slightly from a perfect circle. There's no obvious presence of spiral arms, bars, or strong tidal disturbances. The galaxy appears relatively isolated, without signs of major merging events or significant interactions with nearby galaxies. The light distribution is smoothly varying, lacking distinct substructures.
