The galaxy presents as a spiral type, exhibiting a noticeable disk structure. Spiral arms are clearly visible, emanating from a central bulge. The disk appears relatively face-on to our line of sight. The central bulge seems to be of moderate size, possibly containing a supermassive black hole, given the galaxy's estimated mass. A bar feature is present, though not prominently, bisecting the bulge and influencing the spiral arm structure. The spiral arms exhibit a somewhat flocculent morphology, suggesting ongoing star formation within them. Color gradients within the galaxy suggest varying stellar populations, with bluer regions potentially indicative of younger stars and active star formation, particularly in the spiral arms. The overall morphology is somewhat disturbed, possibly due to minor interactions.
