The galaxy presents as a spiral type, exhibiting a prominent disk structure. Multiple spiral arms are visible, with a moderate winding. The central bulge is moderately sized and shows a yellowish color, indicative of an older stellar population. The spiral arms display a bluer hue, suggesting ongoing star formation. There is evidence of a bar structure, as seen by the slight elongation of the central region. There are minor disturbances to the outer disk, possibly caused by gravitational interactions.
