The galaxy presents as a spiral galaxy, exhibiting a discernible disk structure. The spiral arms are moderately defined, emanating from a central bulge. The bulge appears to be of moderate size, contributing significantly to the overall luminosity of the galaxy. There is no strong evidence of a prominent bar structure within the galaxy's central region. The galaxy displays a slightly inclined orientation with respect to our line of sight. The overall morphology suggests a galaxy that has not experienced any recent major mergers, although minor disturbances or interactions cannot be ruled out. There is strong evidence of spiral arms. 
