The galaxy presents as an elliptical morphology, characterized by a smooth and concentrated light distribution. It exhibits a spheroidal shape with a high degree of roundness. The central region is bright and appears yellowish, suggesting a population of older stars. The luminosity gradually decreases with increasing radial distance from the core. There is no discernible spiral arm structure or prominent dust lanes visible. The overall color profile suggests a relatively passive galaxy, potentially with a low ongoing star formation rate. No significant morphological disturbances or signs of ongoing merger activity are apparent. The galaxy appears to be a relatively isolated system.
