The galaxy presents a primarily disk-like morphology, viewed at an angle that is not quite edge-on. Spiral arm structures are visible, though somewhat diffuse. The winding of these arms appears relatively tight. A central bulge is present, though it does not dominate the galaxy's overall structure. The color profile suggests a mix of stellar populations, with a yellowish hue concentrated towards the bulge, potentially indicative of older, redder stars. The disk exhibits bluer tones, possibly indicating regions of more active star formation. There does not appear to be any major disturbance or clear evidence of a significant merger event impacting the galaxy's morphology. A faint bar structure might be present, though it is not strongly pronounced.
