The galaxy presents as a relatively small, disk-shaped structure. Its orientation suggests it is viewed at a moderately high inclination angle. The central region of the galaxy appears brighter and more diffuse than the outer regions, potentially indicating a significant bulge component. The outer disk exhibits a bluer hue and is composed of a mixture of bright and dark patches, possibly tracing spiral arm segments or dust lanes. There is some asymmetry in the outer regions, which may suggest either tidal interactions or internal activity such as star formation. Overall, the galaxy's morphology is complex, exhibiting characteristics of both smooth and featured components. Evidence suggests it is experiencing some form of disturbance.
