The galaxy presents as a largely smooth and centrally concentrated elliptical morphology. It appears to be relatively featureless, lacking prominent spiral arms or significant dust lanes. There is a slight elongation, but it is mostly rounded in shape. The central bulge dominates the light profile, suggesting an older stellar population. There might be a faint, diffuse halo surrounding the galaxy, but it is not well-defined. The color appears to be relatively uniform across the galaxy, with a subtle reddish hue suggesting it is likely passively evolving. There are no immediately obvious signs of recent major merger activity or ongoing star formation. Any disturbances appear to be minor.
