The galaxy appears to be a spiral type, exhibiting a prominent disk structure. The spiral arms are readily apparent, with an estimated arm count of two dominating. The arms display a medium winding, not overly tight or loose. The color profile suggests a mix of stellar populations; the central bulge appears more yellow, indicative of older, redder stars, while the spiral arms show hints of bluer hues, potentially signifying regions of active star formation with younger, hotter stars. The bulge appears to be of moderate size relative to the overall disk.

The image suggests the galaxy is undergoing some form of interaction or disturbance, with distortions. This disturbance may indicate an ongoing or recent merger event. There is no strong bar structure visible.
