The galaxy presents a clear spiral structure, with two prominent spiral arms easily discernible. The arms appear loosely wound, extending outwards from the central bulge. The central bulge exhibits a moderate size relative to the overall galactic disk. The color gradient suggests a relatively older stellar population concentrated within the bulge, with a shift towards bluer hues in the spiral arms, indicating ongoing star formation. The disk appears somewhat inclined relative to our line of sight, but not completely edge-on. There may be a weak bar structure present within the central region, though this is not definitively clear. There do not appear to be signs of significant merging or major disturbances.
