The galaxy presents a distinct spiral morphology. Two prominent spiral arms are clearly visible, winding moderately around a central bulge. The bulge appears of moderate size, exhibiting a yellowish hue, suggestive of an older stellar population. The spiral arms show a bluer color, indicative of ongoing star formation. The disk of the galaxy is not seen edge-on. A possible interaction or minor disturbance may be present, affecting the overall morphology. The galaxy's form is neither completely smooth nor a clear merger event. There may be evidence of a bar structure, although it is difficult to determine if it is strong or weak.
