The galaxy presents as a centrally concentrated object with a generally smooth appearance. The central region exhibits a bright, yellowish-white core, suggesting an older stellar population. Moving outwards from the core, the light gradually fades into a bluer halo or disk. This halo appears more diffuse and less structured than a typical spiral galaxy, with a largely smooth distribution of light. There is a slight hint of elongation to the structure, with an 'in between' rounded shape rather than a perfectly circular one. Visually, there are no prominent spiral arms or distinct dust lanes. The overall morphology suggests a transition between a pure elliptical galaxy and a spiral, possibly a lenticular galaxy. There are no prominent signs of a major ongoing merger, although a minor disturbance cannot be ruled out due to the subtle asymmetry in the outer regions.
