This galaxy exhibits a spiral morphology. The spiral arms appear somewhat flocculent and asymmetrical, exhibiting a degree of disturbance. There is evidence of ongoing star formation within the arms, indicated by the presence of numerous blue-hued regions likely corresponding to young, hot stars. The central bulge appears relatively smooth, though difficult to resolve clearly in this image. There is some potential indication of a minor tidal interaction or recent merger event, evidenced by the lopsidedness of the spiral structure and slight distortions in the outer regions of the disk. The galaxy's color profile suggests a mixture of stellar populations, with both younger, bluer stars in the arms and older, redder stars in the bulge. Overall, the galaxy appears to be undergoing a period of active star formation, possibly triggered by a recent interaction.
