The galaxy presents a spiral structure. It is oriented approximately face-on relative to our line of sight, allowing for a partial view of its overall morphology. The spiral arms are visible, although they are not sharply defined and appear somewhat flocculent in nature. The winding of the spiral arms is relatively tight. A bar structure is subtly present. There appears to be a moderate central bulge. The galaxy does not appear to be undergoing any major merging events, although there is some irregularity in the arm structure that indicates minor disturbances. Evidence suggests the galaxy exhibits a relatively low star formation rate. The color profile indicates blue tones in the arms, contrasting slightly with the yellower hue of the central bulge, likely due to the presence of younger stellar populations in the arms.
