The object appears to be a spiral galaxy, viewed at a significant inclination. A prominent central bulge is present, with a relatively high concentration of older stars, indicated by its yellowish-white color. Two distinct spiral arms extend from the bulge, exhibiting a loose winding pattern. The disk shows evidence of ongoing star formation, evidenced by the bluish tint observed along the outer edges of the arms. There appears to be some degree of disturbance within the galaxy, though it is unclear if this is due to an interaction. There is no clear evidence of a strong bar structure, but a weak bar cannot be ruled out.
