The galaxy appears as a centrally concentrated object with a generally smooth morphology. The core exhibits a bright, yellowish hue, suggesting a population of older stars. Fainter, diffuse bluish regions are present in the outer portions of the galaxy. These suggest the presence of younger, hotter stars and potentially ongoing, though moderate, star formation. There is a minimal indication of distinct spiral arm structure or a well-defined disk; the overall shape appears largely spheroidal, leaning towards elliptical. No obvious tidal features or signs of major mergers are visible, indicating it is a relatively undisturbed system. Subtle irregularities hint at minor disturbances or possible past interactions.
