The galaxy presents a generally smooth, elliptical morphology. It exhibits a high degree of central concentration, with light appearing most intense towards the galactic nucleus, gradually decreasing with radial distance. The overall shape is close to circular, showing only a slight elongation. There is a hint of minor structural disturbance to one side, potentially indicative of past interactions. The color profile of the galaxy suggests an older stellar population, with a redder hue predominating across the visible spectrum. The Sersic index indicates it is a relatively evolved galaxy.
