The galaxy appears to be a relatively smooth, elliptical-type galaxy. The central region exhibits high surface brightness, gradually decreasing outwards towards the periphery. There's a subtle elongation, it is not perfectly spherical. No distinct spiral arms or bar structures are discernible. It is a relatively isolated galaxy and does not appear to be undergoing any major interactions or mergers, though the outer regions are somewhat irregular. The color distribution suggests an older stellar population, with a concentration of redder hues near the center, possibly indicating a higher density of older, cooler stars in this region. There's also a hint of bluer hues scattered within, suggesting recent or ongoing star formation.
