The galaxy presents a predominantly smooth, elliptical morphology. There is a concentrated central bulge emitting intensely bright, yellowish light, suggesting an older stellar population. Moving outward from the center, the luminous intensity decreases, fading into the background sky. The overall shape is approximately round, showing no visible spiral arm structures or significant disturbances indicative of a recent merger event. The galaxy appears to be relatively isolated and undisturbed. There is some faint emission in the outskirts, suggesting some older star formation.
