The galaxy presents as a relatively smooth, elongated structure, likely a spiral seen edge-on or a lenticular galaxy. There is a subtle color gradient; the central region appears more yellow/orange, possibly indicating an older stellar population. Fainter blue hints at the outer edges suggest the presence of younger stars and ongoing star formation, albeit at a low rate.

The galaxy does not appear to be undergoing any major merging events or significant tidal disturbances, and it displays no major distinct features within its disk.
