The galaxy presents as a spiral type, viewed at an intermediate angle, showing a distinct central bulge with a yellowish hue, indicating a potentially older stellar population in that region. Faint, somewhat diffuse spiral arms extend outwards from the bulge, exhibiting a bluer color suggestive of ongoing star formation. The arms appear somewhat flocculent, lacking a clearly defined structure, and are moderately tightly wound. The galaxy's overall ellipticity suggests a substantial disk component, although the image resolution limits detailed analysis of features such as dust lanes or HII regions within the arms. There is a faint suggestion of a bar-like structure, possibly running through the central bulge, but again image resolution limits detailed examination.
