The galaxy appears as a relatively smooth and rounded object. There is a slight deviation from perfect circularity, suggesting a mild ellipticity. No distinct spiral arms or bar structures are discernible within the galaxy's morphology; the light distribution is centrally concentrated. The galaxy exhibits a general evenness in color, with a hint of redder tones. This could imply a population of older stars. The galaxy seems isolated, showing no strong signs of ongoing or recent major merger events. The overall appearance suggests a mature system.
