The galaxy presents a centrally concentrated morphology, appearing largely smooth with a discernible lack of prominent spiral arm structures or a well-defined disk. The light distribution suggests a roughly elliptical or spheroidal shape, though not perfectly circular, with a slight elongation visible. There is evidence of some internal structure with subtle color variations, suggesting possible variations in stellar populations or dust content. The galaxy exhibits a strong central concentration of light, indicative of a prominent galactic bulge or nucleus. Overall, the galaxy's features are relatively subdued, hinting at an evolved stellar population and potentially reduced levels of ongoing star formation.
