The galaxy presents a largely smooth morphology, with a high degree of central concentration. Its overall shape appears generally rounded, lacking any prominent disk-like structure or spiral arms. The color profile suggests a dominant population of older stars, with a yellowish-white hue in the core. No significant signs of active star formation regions are discernible, the object appears relatively quiescent. There is no evidence of tidal streams, shells, or other features indicating recent or ongoing merger activity; the galaxy appears isolated and undisturbed.
