The galaxy appears as a centrally concentrated object, exhibiting a smooth, spheroidal morphology. It presents with a diffuse golden hue, suggesting a stellar population dominated by older, evolved stars, rather than active star forming regions. There is a slight elongation to the galaxy's shape, however it is largely round. There is no strong evidence of spiral arms, bars, or a distinct disk structure visible within the image. Based on this image, the galaxy appears to be a quiescent, early-type galaxy, likely an elliptical or S0 type. There is little evidence of any tidal features or significant disturbances in its morphology, and there are no obvious signs of a major ongoing merger or recent interaction with another galaxy. It is a relatively isolated galaxy.
