The galaxy presents a clear spiral structure, with tightly wound arms emanating from a central bulge. The bulge appears moderately sized and exhibits a yellowish hue, potentially indicating an older stellar population. The spiral arms themselves display a bluer color, suggesting ongoing star formation. The disk component is prominent, exhibiting a non-edge-on orientation. Evidence suggests a likely lack of a strong bar structure across the galaxy's central region. The overall morphology does not indicate a significant ongoing merger event or major disturbance, although a slight asymmetry in the disk might point towards a minor interaction in its past. Based on color variations, star formation is likely present throughout the spiral arms, but concentrated at the edges of the arms. The galaxy exhibits a smooth appearance overall, with a slight bluer coloration in the outer disk. The overall appearance is that of a fairly luminous galaxy that is well within the local universe.
