The galaxy presents an irregular morphology. A bright, centrally concentrated region is evident, possibly indicating a dense galactic nucleus or bulge. There is an extended diffuse halo surrounding the central region. Evidence of disruption, such as tidal tails or asymmetrical features, are present on the East and West portions of the galaxy. These features are more subtle and could be indicative of a minor merger event, or strong disk features. Overall the galaxy shows a mixture of smooth features alongside signs of disturbance. There are also some features on the Northern portion that point to possible ejections of materials or further disk characteristics. Based on color, stellar populations could vary throughout the galaxy, with younger, bluer stars potentially concentrated in the arms and older, redder stars in the central bulge.
