The galaxy presents a somewhat irregular, diffuse morphology. There is a central, bright concentration of light that appears yellowish-white, suggesting an older stellar population. Fainter, bluish extensions are observed emanating from the central region. These extensions have a patchy, slightly disturbed appearance. The shape of the galaxy appears to be somewhere between round and elongated. Overall, the galaxy exhibits signs of potential gravitational disturbance or interaction, with the presence of disturbed, faint features. The color gradients suggest on-going, albeit possibly subdued, star formation in the outer regions, contrasted by an older stellar population in the core.
