The galaxy presents as a well-defined, elliptical structure with a bright, concentrated central bulge that fades gradually towards the outer regions. The overall color gradient suggests a higher concentration of older stellar populations within the bulge, exhibiting a yellowish-red hue, while the outer disk shows slightly bluer tones, possibly indicating younger stars. There is no distinct dust lane or spiral arm structure visible in the image, supporting a classification as an early-type galaxy. The galaxy has a smooth appearance, hinting at a lack of recent major merger events. The morphology is approximately 7 arcseconds across, and exhibits an elongated profile.
