The galaxy presents as a spiral type, exhibiting a prominent disk structure with a central bulge. Two spiral arms dominate the galactic structure, displaying a somewhat open winding pattern. A distinct bar-like feature appears to traverse the center of the bulge. The bulge itself appears moderate in size relative to the overall disk. The disk presents a mottled texture, suggestive of star-forming regions. No evidence of major mergers or significant disturbances is observed, though some minor asymmetry in the outer regions might indicate past interactions. The orientation is face-on relative to our line of sight.
