The galaxy presents as a roughly circular, unresolved object. It appears to have a smooth, concentrated morphology, lacking any discernible spiral arms or distinct features like bars. The color profile suggests a higher concentration of older stellar populations, exhibiting a reddish-yellow hue. There is a subtle hint of a potential minor disturbance or irregularity in its form, specifically a marginal shift in the radial symmetry of its light distribution. The galaxy does not appear to be undergoing a major merger event but has a small chance of some sort of disturbance.
