The galaxy presents as a luminous, centrally concentrated object, exhibiting a generally smooth morphology. There is a subtle elongation of the galaxy's overall shape, deviating slightly from perfect circularity; a slight cigar-shaped quality is visible. The central region displays a notably brighter, yellowish-white hue, suggesting a concentration of older stellar populations or a possible active galactic nucleus. Fainter, reddish tinges are observed in the surrounding regions, indicating the presence of cooler stars or dust. A degree of asymmetry or disturbance is perceptible, possibly indicative of minor gravitational interaction with another galaxy. There is evidence of past or ongoing merging activity.
