The galaxy appears to be a spiral galaxy, however there are some signs of disturbance, indicating a potential interaction with another galaxy. The morphology is somewhat irregular, with an ill-defined and asymmetrical structure. 

The central bulge is not particularly pronounced and appears relatively smooth. The disk exhibits a clumpy structure with the beginning of visible arms. The arms are diffuse and not tightly wound. There is a noticeable blue color gradient in parts of the galaxy, indicative of ongoing star formation, however, the overall star formation rate appears subdued. Some regions exhibit a more reddish hue, suggesting the presence of older stellar populations. 

There are some indications of possible tidal features or distortions in the outer regions of the galaxy, further suggesting an interaction or past merger event. However, a significant portion of the galaxy exhibits a relatively smooth appearance, possibly due to it being an older event.
