This galaxy exhibits a distinct spiral structure, although the arms appear somewhat diffuse. The central bulge is prominent, exhibiting a yellowish hue, suggesting a population of older stars. The disk shows patches of bluer light, indicative of ongoing star formation. There is an indication of a tidal disturbance in the structure, possibly from an ongoing or recent merger event. There are noticeable distortions in the spiral arm structure. There is no obvious central bar feature. The galaxy is viewed at an intermediate angle; it is not seen face-on, nor is it edge-on.
