The galaxy presents a largely smooth, elliptical morphology. Its color profile suggests an older stellar population. There is a concentration of light toward the center, indicative of a galactic bulge. No spiral arm structures are readily apparent. There is minimal evidence of ongoing star formation, based on the absence of significant blue emission regions. The galaxy appears relatively isolated, with no indications of ongoing or recent merger activity or tidal disturbances. It exhibits a rounded shape, lacking any clear asymmetry. The lack of prominent dust lanes supports its classification as an early-type galaxy.
