The galaxy presents as a centrally concentrated, elliptical-like structure. The light is a generally smooth distribution with a high degree of central concentration, indicative of an older stellar population. The primary color is a yellow-orange hue, supporting the presence of evolved stars and a relative lack of ongoing, high-mass star formation. There may be some minor disturbances or a tidal feature on the upper left side of the galaxy, which might suggest a past or ongoing interaction with another galaxy. Overall, the galaxy appears to be relatively isolated and undisturbed, displaying a simple spheroidal morphology.
