The galaxy presents a spiral morphology, observed at a slight inclination to our line of sight. Two prominent spiral arms emanate from a central bulge, wrapping around approximately one-half rotation. The spiral arms exhibit a medium winding, appearing neither tightly wound nor overly diffuse. The central bulge appears moderate in size, exhibiting a yellowish hue, which could indicate an older stellar population. The spiral arms are bluer in color, suggesting the presence of younger, hotter stars. The arms display some degree of patchiness and granularity, which may be indicative of active star formation regions. No strong bar feature is visible. The galaxy doesn't appear to be undergoing any major merger events or exhibiting signs of significant tidal disturbances, though there may be some subtle distortion in the outer regions of the disk.
