The galaxy presents as a generally smooth, centrally concentrated object with a radial gradient in luminosity. The core region appears bright and yellowish, suggesting a population of older stars, possibly with some dust obscuration. The outer regions fade gradually, displaying a slightly redder hue compared to the core, hinting at the presence of a somewhat younger, though still relatively old, stellar population. The shape approximates a spheroid, with a high degree of circularity. There is no obvious evidence of spiral arms or a prominent disk structure. No significant tidal disturbances or signs of ongoing merger activity are readily apparent in the morphology. Based on its overall appearance, this is likely an elliptical or lenticular galaxy, with a considerable mass. The apparent lack of significant star formation and a smoothly distributed light profile are consistent with a galaxy that has largely exhausted its gas supply and experienced minimal recent interactions.
