The galaxy appears as an elliptical-like structure with a smooth, somewhat diffuse morphology, exhibiting minimal distinct features. It presents a yellowish-white hue, suggesting an older stellar population. The light distribution is centrally concentrated, with a gradual decrease in intensity towards the edges. There is evidence of two central points or perhaps a merging system, appearing to be in its late stages. There is no obvious spiral arm structure or dust lane visible in this image, further supporting its smooth, spheroid-like nature. There is a subtle irregularity to the shape, hinting at potential gravitational interaction or past merger events.
