The galaxy appears to be a generally smooth object, elliptical in shape. The central region exhibits a high degree of luminosity, characterized by a yellowish-white hue, suggesting a population of older stars. The light gradually diffuses outwards from the center, transitioning to a reddish-orange color in the outer regions. This suggests the presence of an aging stellar population and a low rate of current star formation. The overall form shows high central concentration. There is no obvious spiral structure visible. There appears to be a small, more compact, possibly related object or foreground object to the left of the main galaxy.
