The galaxy presents as a spiral type, exhibiting a notable disk structure. Two prominent spiral arms are clearly visible, tracing a relatively tight winding pattern around a central bulge. The bulge appears relatively small in comparison to the overall disk size. The galaxy exhibits a slight asymmetry, with some possible minor disturbances or tidal features possibly indicating past or ongoing interaction. The color profile suggests active star formation, particularly within the spiral arms. The overall morphology is indicative of a reasonably evolved spiral galaxy with a well-defined structure. There is no clear evidence of a strong bar feature.
