The galaxy presents as a single, relatively smooth and symmetrical entity. Its morphology appears elliptical, exhibiting a high degree of central concentration with a radial decrease in luminosity. The core region displays a bright, yellowish-white hue, suggesting a population of older, evolved stars. Moving outward from the core, the color shifts towards a slightly redder tone, hinting at the presence of a mix of stellar populations or dust absorption. No distinct spiral arms, bars, or other prominent features are discernable, consistent with an early-type classification. There is no obvious morphological disturbance to suggest ongoing or recent merger activity. The galaxy exhibits a defined edge, further supporting the conclusion that it is an elliptical galaxy.
