The galaxy presents as a largely smooth, elliptical structure. The central region exhibits a concentrated, bright yellow-gold hue indicative of a substantial population of older stars and minimal dust obscuration. Moving outward from the core, the color transitions to a redder, fainter, and less concentrated distribution, suggesting a declining density of stars and possibly some redder stars in the outer regions. There may be some slight minor disturbances occurring within the galaxy, possibly due to an ongoing or recent minor merger, but generally is a singular non disturbed object. The galaxy appears mostly round.
