This galaxy appears to be a spiral galaxy viewed at a high inclination, nearing edge-on. The central bulge is bright and prominent, exhibiting a roughly circular shape. The galactic disk appears to be significantly disrupted. There is evidence of some irregularities and potential tidal features around the outer regions of the galaxy, especially visible along one side. There is some minor evidence of disturbance on the opposite side, though it is fainter and less pronounced. These could indicate either a past or ongoing interaction with another galaxy. The galaxy exhibits a bluer color in its disk and the bulge, which can indicate younger star formation, especially when compared to the halo surrounding it. Overall the morphology suggests a galaxy undergoing some level of disruption, though perhaps not a full major merger. 
