The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in surface brightness outward from the core. The galaxy presents a round morphology. There's little evidence of spiral arms or a significant disk component. The color profile is relatively uniform across the galaxy, suggesting a lack of significant ongoing star formation. It appears to be a fairly evolved system. Faint, diffuse light extends beyond the main body, suggesting a stellar halo. No signs of major disturbances or merging events are visible.
