The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. It appears largely featureless, lacking any discernible spiral arms or significant dust lanes. The light profile suggests a uniformly distributed stellar population, with a gradual decrease in brightness from the core outwards. The color is generally blue-white, indicating the presence of relatively young, hot stars and ongoing star formation, albeit at a moderate rate. There is no evidence of recent or ongoing major mergers, although subtle asymmetries could indicate minor disturbances or past interactions. The overall shape is quite round, showing only minor deviations from a perfect ellipse.
