The galaxy presents as a largely featureless, elliptical morphology. Its overall color is a yellowish-orange hue, suggesting an older stellar population with minimal recent star formation. There is a smooth, gradual decline in luminosity from the central region outwards, lacking distinct spiral arms or prominent dust lanes. The light distribution is concentrated towards the center, indicating a dense galactic nucleus. The shape appears mostly round, with little sign of elongation or asymmetry, implying a relaxed dynamical state. The absence of any obvious tidal features or distortions suggests it is not currently undergoing a major merger event, although some minor interactions in the past cannot be ruled out. The galaxy appears relatively isolated, with no obvious close companions that might be influencing its morphology.
