The galaxy presents a complex morphology suggestive of an ongoing or recent merger event. The core of the galaxy appears relatively smooth and centrally concentrated, exhibiting a yellowish-white hue indicative of an older stellar population. A distinct, bluish extension emanates from the main body, potentially representing tidal features or disrupted spiral arm structures resulting from gravitational interactions. There may be some dust obscuring the central region as well. The overall shape is somewhat irregular, deviating significantly from a simple elliptical or spiral form. Overall, the galaxy appears to be in a state of considerable dynamical disturbance.
