The galaxy presents as a spiral type, with a noticeable disk structure and distinct spiral arms. The spiral arms appear grand in design, extending outwards from a central bulge.

The bulge is moderately sized, exhibiting a yellowish-orange hue suggestive of an older stellar population. The disk displays a bluer tint, indicating the presence of younger stars and active star formation regions within the spiral arms. Patches of increased brightness and color variation are observable throughout the disk, possibly regions of HII emission nebulae.

The galaxy is inclined to our line of sight, providing a less than ideal view of the disk. Some indication of a possible bar structure within the central region is evident, though not particularly pronounced. There are no readily apparent signs of any major ongoing merger event, although some subtle asymmetries within the spiral arm structure cannot be ruled out as indicators of past minor interactions.