The galaxy appears to be a relatively smooth, elliptical galaxy, with no obvious spiral arm structures or dust lanes visible. The core of the galaxy presents a concentrated brightness, suggesting a high stellar density. Its shape is somewhere between round and slightly elongated. There are no distinct tidal tails or other morphological disturbances to indicate a recent major merger event, though a very slight asymmetry is visible along its edges. The color profile of the galaxy exhibits a gradient, appearing more yellow/red in the central regions, suggesting an older stellar population. The outer regions have a slightly bluer tint suggesting a younger stellar population.
