The galaxy presents a largely smooth morphology, with minimal discernible features such as spiral arms or a distinct bar structure. Its overall shape appears roughly circular, exhibiting a high degree of central concentration. Color gradients suggest a concentration of older stellar populations towards the galactic center, which glows with a yellow hue. Fainter, bluish regions are observed in the outer reaches, possibly indicative of younger, hotter stars, though these features are not prominent. There is little evidence of significant ongoing merger activity or tidal disturbances in the image. The galaxy's light profile smoothly diminishes with increasing radius, implying a well-mixed stellar population.
