The galaxy presents as a somewhat elongated structure with a diffuse, smooth appearance. There is a noticeable color gradient, with the central region appearing more yellow-red, suggesting an older stellar population, while the outer regions show hints of bluer hues, possibly indicating regions of ongoing or recent star formation. The overall morphology is likely that of a disk galaxy, though any distinct spiral arms are not visible given the data available. There are signs of some kind of gravitational disturbance, as the main galaxy body appears to be asymmetric and distorted. This could potentially be due to a minor merger event with a smaller galaxy. A small irregular object is visible nearby, which may be interacting with the larger galaxy.
