This galaxy exhibits a distinct spiral structure, with moderately defined arms. The arms appear somewhat flocculent, rather than grand design. The central bulge is prominent and appears yellowish, suggesting an older stellar population. The disk shows a bluer hue, likely indicative of more recent star formation. A bar-like structure appears to be present, extending through the central region. Overall, the galaxy doesn't appear to be undergoing any major merging activity, with only slight disturbances in the spiral arm structure.
