The observed galaxy presents a distinct spiral morphology. Two prominent spiral arms are discernible, exhibiting a tightly wound structure around a central bulge. The bulge appears moderate in size, contributing significantly to the overall luminosity of the galaxy's core. The disk of the galaxy is viewed nearly face-on, allowing for a clear observation of the spiral arm structure. There is a subtle suggestion of a bar-like feature extending across the central region, although it is not strongly defined. A significant portion of the galactic disk exhibits a smooth, homogeneous appearance, while other regions show features indicative of active star formation. There appears to be no major disturbance or ongoing merger event drastically altering the galaxy's overall structure, though the galaxy does not appear to be perfectly isolated.
