The galaxy presents as a spiral type, observed at an intermediate inclination. The disk component exhibits spiral arms, somewhat tightly wound, though a precise count is difficult to ascertain due to the inclination and resolution. A prominent central bulge is noticeable, exhibiting a yellowish hue, suggestive of an older stellar population. The spiral arms display a bluer color, indicative of ongoing star formation. There is a hint of a bar structure present. No major merging is seen, but some minor disturbances in the disk could suggest minor interactions. Overall, the galaxy exhibits a classic spiral morphology with evident star formation activity within its arms.
