The galaxy presents as a spiral type, viewed at an oblique angle relative to its disk. The spiral arms are discernible, though the inclination obscures a clear view of their full extent and structure. There is evidence of a central bulge of moderate size. It displays a somewhat clumpy morphology, potentially indicating active star formation regions within the arms. The presence of a bar structure within the central region is suggested. The overall light distribution indicates some disturbance and possible ongoing interaction or minor merger. A portion of the galaxy's structure could also be interpreted as a tidal feature or disrupted arm segment. There is also a smooth component, which may be a stellar halo. The color gradient suggests a range of stellar populations, with bluer regions indicating younger stars and redder regions representing older stellar populations or dust obscuration.
