This galaxy presents a generally smooth morphology with a somewhat concentrated central region. A subtle disk-like structure is possibly present, though features are poorly defined. The galaxy exhibits a color gradient, transitioning from a bluer hue in its core to redder tones in its outer regions, suggesting a potential gradient in stellar populations, dust content, or redshift across the galaxy. A faint indication of minor disturbance may be present. Overall, the galaxy appears relatively isolated, with no clear signs of a major ongoing merger, though the subtle disk and possible disturbances suggest a more complex history.
