The galaxy presents a generally smooth morphology, with a high degree of central concentration. The light profile suggests a spheroid-dominated system. The central region exhibits a yellowish hue, indicative of an older stellar population, while the outer regions show a slightly bluer color, possibly indicating the presence of some younger stars or ongoing star formation, albeit at a relatively low rate. The overall shape appears largely circular, showing little to no discernible disk structure. There is no strong evidence of major disturbances or recent merger activity in the system's overall structure.
