The galaxy presents as a single object with some internal structure. The core region appears roughly circular, with the overall morphology tending toward round. Light distribution suggests that the center is not uniform, with some possible disturbance.

A distinct blue component is visible, suggesting the presence of hotter, younger stars. The outer regions exhibit a redder hue compared to the inner regions.

There appears to be some evidence of tidal features or minor disturbances in the galaxy's morphology, indicating past interactions with another object. The galaxy doesn't show any signs of large-scale spiral arms or a well-defined disk structure. There is a hint of asymmetry.
