The galaxy presents a largely smooth, elliptical morphology. It appears relatively featureless with a high degree of central concentration, suggesting an older stellar population. The galaxy exhibits a yellowish hue, consistent with older stars. The radial light profile suggests a gradual decline in brightness from the center outwards. There may be some evidence of a slight disturbance in its overall structure. Based on its overall appearance, this is likely a galaxy with suppressed star formation.
