The galaxy presents as a spiral type, viewed at a slight angle relative to edge-on. There is evidence of loosely wound spiral arms extending from a central bulge. The bulge appears moderate in size relative to the overall galactic disk. The color distribution suggests active star formation, indicated by the bluer hues within the arms. The overall structure appears largely undisturbed, showing no signs of ongoing major merging activity, though there may be minor irregularities. A faint bar structure can be observed within the central region, though it is not particularly prominent.
