The galaxy presents as a spiral type, exhibiting distinct, although somewhat diffuse, spiral arms emanating from a central bulge. These arms appear to be grand design with two primary arms and a medium winding. The bulge component seems moderate in size, contributing significantly to the overall luminosity of the galaxy. The disk appears prominent, with a near face-on orientation relative to the observer. There is no strong visual indication of a bar structure bisecting the bulge. The galaxy displays a notable degree of internal structure within the arms, with indications of star-forming regions. There are no obvious signs of any major merging activity, although there may be minor irregularities within the disk. Overall, the system appears to be a relatively undisturbed spiral galaxy.
