The galaxy presents as a centrally concentrated, elliptical-like object. It displays a smooth, almost featureless morphology, lacking prominent spiral arms or a distinct bar structure. The light distribution indicates a high degree of central concentration with a gradual decline in surface brightness outward from the core. The galaxy exhibits a roughly spherical shape, showing minimal deviation from a circular isophote. There is no evident tidal interaction or merging activity detected in the image. The object's color indices suggest a population of older, redder stars, indicative of a low star formation rate.
