The galaxy presents an overall roughly elliptical morphology. The core region exhibits a bright, concentrated luminosity, suggesting a dense stellar population or active galactic nucleus. The surrounding structure appears relatively smooth, with a subtle indication of diffuse, extended features around the primary luminous core. The overall color gradient appears to shift from bluer tones toward the center, to redder hues in the outer regions. There is minor visual evidence for disturbances in the overall structure of the galaxy. Faint, subtle irregularities or asymmetries are seen in the distribution of luminosity.
