The galaxy appears as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, which emits strongly across the observed bands, suggesting a high density of older stellar populations. There may be a weak disk. The overall color profile indicates a relatively mature galaxy, with possible ongoing, but limited star formation. There may be very minor disturbances in the galaxy shape, but not significant enough to qualify as an active merger. The galaxy is of intermediate size.
