The galaxy presents as a relatively smooth, elliptical-like object. It appears to be an early-type galaxy, likely an elliptical, with a high degree of central concentration. There is a smooth, gradual falloff in surface brightness from the core outward, with a subtle elongation in its overall shape, suggesting an intermediate sphericity. There is no prominent disk structure observed. The galaxy’s light profile indicates an older stellar population and low levels of ongoing star formation. Faint blue light is present, perhaps from the remnants of star formation. There does not appear to be any evidence of recent major mergers or tidal disturbances.
