The galaxy presents as a spiral type, exhibiting a well-defined disk structure. Two prominent spiral arms are visible, exhibiting a winding pattern of moderate tightness. The central bulge is moderately sized, contributing significantly to the overall luminosity. A bar structure is apparent, though difficult to discern due to the image quality. There are hints of internal structure within the spiral arms, possibly indicating areas of active star formation. The galaxy does not appear to be undergoing any major mergers, though there are very minor signs of tidal disturbance.
