The galaxy presents a generally smooth, elliptical morphology. There is a high degree of central concentration with the light profile decreasing radially outwards. The core exhibits a yellowish hue, suggesting an older stellar population. Fainter, bluer light surrounds the core region, hinting at more recent, albeit modest, star formation activity. The galaxy's structure appears relatively undisturbed, with no obvious signs of tidal features or ongoing major merger events. There are no visible spiral arm structures within the galaxy. The overall shape of the galaxy is roughly round. There appears to be little to no dust present.
