The galaxy exhibits a somewhat distorted morphology, suggestive of an ongoing or recent interaction. A prominent disk structure is visible, but it appears tilted nearly edge-on from our perspective. The central bulge is quite luminous and exhibits a yellowish hue, potentially indicating an older stellar population. Evidence of disruption is visible, with what appear to be tidal features extending outwards from the main galactic body in the North direction. These features suggest gravitational interaction with another galaxy or past merger events. The disk itself shows some signs of internal structure. Overall, the galaxy does not appear to be a quiescent system, and its current form is likely the result of dynamic processes.
