The galaxy presents as a centrally concentrated object with a relatively smooth overall appearance. It exhibits a somewhat elongated, cigar-like shape, with a noticeable color gradient from the core outwards. The central region displays a whitish-yellow hue, potentially indicating an older stellar population. Moving outward from the center, a faint blueish tint is observed, which may suggest the presence of some younger stars, implying ongoing or recent star formation, albeit at a low level. There is no apparent indication of strong spiral arms or a distinct disk structure. It is categorized as a relatively massive galaxy. There is no indication of a major merger occurring, but there may be minor disturbance occurring.
