The galaxy presents as a relatively compact, elliptical structure, exhibiting a smooth, featureless morphology. Its light distribution suggests a high degree of central concentration, with a gradual decrease in luminosity outward from the core. The galaxy's overall color appears reddish-orange, indicative of an older stellar population. The absence of distinct spiral arms or other prominent features suggests a lack of significant ongoing star formation. There may be some minor gravitational disturbance based on its asymmetry. 
