The galaxy presents a generally smooth and elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct disk structure. The color gradient suggests a population of older stars, exhibiting a reddish-yellow hue concentrated towards the galactic center. There is little evidence of recent or ongoing star formation, which is consistent with the smooth, spheroidal appearance. The object shows a high degree of circularity, with a lack of any significant tidal distortions or merging features to suggest recent interactions. There may be some minor disturbances present, but overall the galaxy appears relatively relaxed and undisturbed. The luminosity profile indicates a centrally concentrated brightness distribution, with intensity decreasing gradually with increasing radial distance.
